The galaxy presents a somewhat irregular morphology. The primary body of the galaxy appears smooth, with a concentrated central bulge. There is evidence of a possible disk structure or extended feature. The bluer color suggests ongoing star formation, although the relatively smooth appearance indicates that star formation might be distributed or less intense. There are hints of possible disturbances or tidal features. It is possible that the galaxy is undergoing a minor merger event, or has experienced one in the past. Alternatively, it could be a disk galaxy undergoing some sort of tidal interaction with another nearby galaxy. The galaxy has a significant mass estimate and a relatively low star formation rate.
