Either its axial inclination is a bit over 90 degrees and its rotation is direct, or it's a bit less than 90 degrees and the rotation is retrograde. The problem is that you need to draw a dividing line somewhere because in case like Venus there is a dispute that the rotation is indeed retrograde or not a direct rotation with an inclination of 180 degrees. Uranus is primarily composed of rock and various ices, with only about 15 percent hydrogen and a little helium. It is in many ways similar to the cores of the great Jupiter and Saturn but rather that its material is more or less uniformly distributed. Like other gas planets, Uranus has bands of clouds that blow around rapidly, but they are extremely faint, visible only with radical image enhancement of the Voyager 2.
Recent observations show that larger and more pronounced streaks appear on the planet.
The blue color on Uranus is the absorption of red light by methane in the upper atmosphere. There may be colored bands like Jupiter's but they are hidden from the view by overlaying methane layer. Also like other gas planets, Uranus has rings. As like Jupiter, they are dark. But like Saturn's rings, it is composed of fairly large particles ranging up to 10 meters in diameter in addition to fine dust.