The galaxy appears as a somewhat rounded, centrally concentrated object. The light profile suggests it's generally smooth in appearance. There is evidence of a possible interaction or merger event ongoing. There seems to be a disturbance or asymmetry in its structure, perhaps indicating minor tidal interactions or a past merger. The object exhibits a color gradient, with the central region appearing more reddish-yellow than the outer regions, which have a bluer tinge. The estimated size is consistent with a massive galaxy. Its specific star formation rate indicates that the galaxy's star formation activity is suppressed. Overall, this appears to be a massive, relatively quiescent galaxy potentially in the late stages of a merger.
