The galaxy presents as a disk galaxy, observed at a slight angle from face-on. Spiral arm structures appear to be present but are not sharply defined; they are somewhat flocculent in nature. There is a central bulge, which is not particularly dominant, and appears to be fairly compact, with a moderate concentration of light. The disk itself demonstrates a range of stellar populations as indicated by variations in color. The overall form of the galaxy is somewhat disturbed, potentially indicating a past or ongoing interaction, or possibly internal dynamic processes. The galaxy presents some clumpy features, and is relatively large and massive with moderate levels of ongoing star formation activity.
