Question: What British astronomer and composer discovered the barred spiral galaxy known as "NGC 4454"?

Context articles: William Herschel
NGC 3190
NGC 4319
NGC 7331
NGC 7479
NGC 2207 and IC 2163
NGC 3344
NGC 4454
NGC 4444
Intermediate spiral galaxy

Frederick William Herschel, (German: "Friedrich Wilhelm Herschel" ; 15 November 1738 – 25 August 1822) was a British astronomer and composer of German and Czech-Jewish origin, and brother of fellow astronomer Caroline Herschel, with whom he worked.
 Born in the Electorate of Hanover, Herschel followed his father into the Military Band of Hanover, before migrating to Great Britain in 1757 at the age of nineteen.
NGC 3190 is a spiral galaxy with tightly wound arms and lying in the constellation Leo.
 It was discovered by William Herschel in 1784.
 NGC 3190 is member of Hickson 44 galaxy group, estimated at around 80 million light years away, and consisting of four galaxies in a tight group - NGC 3193 is fairly featureless, NGC 3187 is a dim but striking spiral galaxy and NGC 3185 has a barred spiral structure with an outer ring.
NGC 4319 is a face-on barred spiral galaxy located about 77 million light years away in the constellation Draco.
 The morphological classification is SB(r)ab, which indicates it is a barred spiral with an inner ring structure and moderate to tightly wound arms.
 It is situated in physical proximity to the galaxies NGC 4291 and NGC 4386, with X-ray emissions from the intervening gap indicating NGC 4319 and NGC 4291 may be interacting.
 NGC 4319 has a much higher proportion of ionized hydrogen compared to the Milky Way galaxy.
NGC 7331 (also known as Caldwell 30) is a unbarred spiral galaxy about 40 e6ly away in the constellation Pegasus.
 It was discovered by William Herschel in 1784.
 NGC 7331 is the brightest member of the NGC 7331 Group of galaxies.
 The other members of the group are the lenticular or unbarred spirals NGC 7335 and 7336, the barred spiral galaxy NGC 7337 and the elliptical galaxy NGC 7340.
 These galaxies lie at distances of approximately 332, 365, 348 and 294 million light years, respectively.
 In both visible light and infrared photos of the NGC 7331, the core of the galaxy appears to be slightly off-center, with one side of the disk appearing to extend further away from the core than the opposite side.
NGC 7479 (also known as Caldwell 44) is a barred spiral galaxy about 105 million light-years away in the constellation Pegasus.
 It was discovered by William Herschel in 1784.
 Supernovae SN 1990U and SN2009jf occurred in NGC 7479.
 NGC 7479 is also recognized as a Seyfert galaxy and a Liner undergoing starburst activity not only on the nucleus and the outer arms, but also across the bar of the galaxy, where most of the stars were formed in the last 100 million years.
 Polarization studies of this galaxy indicate that it recently underwent a minor merger and that it is unique in the radio continuum, with arms opening in a direction opposite to the optical arms.
 This feature, along with the asymmetrical arms of the galaxy and the intense star formation activity are attributed to a merger with a smaller galaxy.
 This galaxy is similar in both size and morphology to the barred spiral NGC 1300.
NGC 2207 and IC 2163 are a pair of colliding spiral galaxies about 80 million light-years away in the constellation Canis Major.
 Both galaxies were discovered by John Herschel in 1835.
 The larger spiral, NGC 2207, is classified as an intermediate spiral galaxy exhibiting a weak inner ring structure around the central bar.
 The smaller companion spiral, IC 2163, is classified as a barred spiral galaxy that also exhibits a weak inner ring and an elongated spiral arm that is likely being stretched by tidal forces with the larger companion.
 Both galaxies contain a vast amount of dust and gas, and are beginning to exhibit enhanced rates of star formation, as seen in infrared images.
 So far, four supernovae have been observed in NGC 2207:
NGC 3344 is a relatively isolated barred spiral galaxy located 22.5 million light years away in the constellation Leo Minor.
 This galaxy belongs to the group known as the Leo spur, which is a branch of the Virgo Supercluster.
 NGC 3344 has the morphological classification (R)SAB(r)bc, which indicates it is a weakly barred spiral galaxy that exhibits rings and moderate to loosely wound spiral arms.
 There is both an inner and outer ring, with the prominent arms radiating outward from the inner ring and the slightly elliptical bar being situated inside.
 At the center of the bar is an HII nucleus with an angular diameter of about 3″.
NGC 4454 is a barred spiral galaxy located about 123 million light-years away in the constellation of Virgo.
 NGC 4454 was discovered by astronomer William Herschel on April 17, 1784.
NGC 4444 is an intermediate spiral galaxy in the constellation Centaurus.
 The morphological classification places it midway on the continuum between a barred spiral (SB) and an unbarred spiral (SA), with an inner region that lies between a ring-like ("r") and a purely spiral form ("s"), and medium- ("b") to loosely wound ("c") outer spiral arms.
 This makes it a hybrid ringed, barred spiral galaxy.
 It has an angular size of 2.4 × 1.6 arcminutes and the estimated mass "M" is given log "M" = 9.76, yielding 5.8 billion solar masses.
An intermediate spiral galaxy is a galaxy that is in between the classifications of a barred spiral galaxy and an unbarred spiral galaxy.
 It is designated as SAB in the galaxy morphological classification scheme.
 By definition, a galaxy is a congregation of stars held together by gravity.
 The first intermediate spiral galaxy discovered is the Milky Way, by Galileo, in 1610.
 He was the first person with a telescope powerful enough to make such a discovery.
 Before Galileo, it was thought that all bright objects in the sky were either the planets in the Solar System, moons, comets, or stars.
 Until the beginning on the twentieth century, astronomers did not know the size of the Universe, but speculated it to be about as big as the Milky Way.
 In 1920, at the National Academy of Science, there was a big debate between Harlow Shapley and Heber D. Curtis on whether nebulae are small globular clusters surrounding the Milky Way, or separate galaxies located farther away.
 Nothing was resolved at the debate; neither side was able to provide conclusive evidence to prove their side correct over their opponent.
 In 1923, Edwin Hubble resolved the matter with a photograph that he took of the Andromeda Galaxy.
 What he found in his photograph was a very bright light source pulsing at a certain rate, a Cepheid variable, located outside the Milky Way.
 This can be used to determine the distance to it.
 Hubble proved that the Universe was full of galaxies, and disproved that the Milky Way was the extent of the Universe.
 There are many types of galaxies in the Universe, elliptical, barred spiral galaxies; they vary in shape and size, but on average spiral galaxies are the most abundant.