The galaxy presents a disk-like morphology, viewed at an angle that suggests it is close to face-on. Prominent spiral arms emanate from a central bulge. The spiral arms appear relatively flocculent with clear areas of intense star formation with pockets of redder more concentrated star formation. The winding of the spiral arms is somewhat loose. A small amount of disruption suggests a merger or other interaction. The central bulge exhibits a moderate size relative to the overall galactic disk. No bar structure is readily discernible. The overall appearance suggests a spiral galaxy with ongoing star formation activity within its disk and spiral arms.
