  The MGRO J2019+37 region is one of the brightest sources in the sky at TeV
energies. It was detected in the 2 year HAWC catalog as 2HWC J2019+367 and here
we present a detailed study of this region using data from HAWC. This analysis
resolves the region into two sources: HAWC J2019+368 and HAWC J2016+371. We
associate HAWC J2016+371 with the evolved supernova remnant CTB 87, although
its low significance in this analysis prevents a detailed study at this time.
An investigation of the morphology (including possible energy dependent
morphology) and spectrum for HAWC J2019+368 is the focus of this work. We
associate HAWC J2019+368 with PSR J2021+3651 and its X-ray pulsar wind nebula,
the Dragonfly nebula. Modeling the spectrum measured by HAWC and Suzaku reveals
a $\sim$7 kyr pulsar and nebula system producing the observed emission at X-ray
and ${\gamma}$-ray energies.
