The galaxy presents as a relatively small, somewhat diffuse object. It exhibits a predominantly smooth morphology, with a bright, centrally concentrated core or bulge. There is evidence of a disk structure around the core. The disk appears generally smooth and flocculent. Some minor disturbances are present, possibly indicative of past minor mergers. Overall, the galaxy appears to be a relatively low mass system. Star formation is detected at a low rate. The color profile suggests that the galaxy is composed primarily of older stellar populations. There is a slight blue tint that indicates there is very little young star formation. Overall, it looks like the galaxy is a transition from active to more quiescent star formation.
