The galaxy presents a largely smooth, rounded morphology. A bright, centrally concentrated bulge dominates the visual appearance. The color profile suggests an older stellar population in the bulge, appearing more yellow-red in composite color. Fainter, extended features, possibly indicating a disk component are present, with slightly bluer tints that may indicate more recent star formation regions. The disk appears to be undergoing some minor tidal disruption, or potentially has a companion merging with it. Overall, the galaxy is likely a massive system, with signs of suppressed star formation and ongoing interaction with another galaxy.
