This galaxy exhibits a generally disk-like morphology, though appearing somewhat disturbed. A central bulge is present, exhibiting a bright, concentrated luminosity possibly indicative of an active galactic nucleus or a high density of stars. Moving outward from the center, the disk appears to be asymmetric. There is evidence of clumpy star formation within the arms of the disk, signified by areas of bright, concentrated light in the "g" band. The asymmetry could be due to a minor gravitational interaction, as indicated by distortions in the overall shape of the disk. A possible tidal tail extends from one side of the galaxy.
