This galaxy appears to be relatively compact and centrally concentrated. There is a bright core, possibly indicative of an active galactic nucleus or a dense stellar population. The overall morphology is somewhat amorphous. There is some evidence of disruption or tidal features, with extensions of fainter material emanating from the main body of the galaxy. These extensions suggest potential interaction with a companion galaxy or past merger event. Overall, the galaxy has a distorted shape and a non-uniform surface brightness distribution, possibly indicating that it is undergoing or has recently undergone a merger.
