The galaxy exhibits a clear spiral structure with two prominent arms that are tightly wound around the central bulge. These spiral arms suggest ongoing star formation, indicated by the presence of bluer regions within them. The galaxy's disk appears to be inclined at an angle relative to our line of sight, and is elliptical. There is a small bulge in the galaxy. The overall shape seems relatively undisturbed, indicating a stable configuration without any major merging events. 
