The galaxy presents as a single, moderately luminous entity with a notable red hue. The overall form appears somewhat disturbed, possibly indicative of an ongoing or recent merger event. There is a prominent bulge, with evidence of extended tidal features or asymmetries. The luminosity profile suggests that the galaxy is dominated by an older stellar population. Star formation rates are low, consistent with an aging galaxy. The morphology is intermediate in roundness. Signs of a merging partner seem distinct. There are some indications of disturbances, but appear to be on the minor side. However, the high merger fraction indicates a substantial likelihood that this galaxy is in some stage of merging with another galaxy.
