The galaxy appears to be a smooth, elliptical type, displaying a centrally concentrated bulge that diminishes in luminosity toward its outer edges. The galaxy exhibits a subtle elongation, appearing somewhat disk-like. There are no signs of spiral arms, dust lanes, or significant irregularities. The light distribution appears largely uniform and smooth across the galaxy's surface, with a color gradient suggesting that younger, bluer stars are less concentrated towards the center than older, redder stars. There is no obvious indication of any major ongoing or recent merging activity, though subtle asymmetries may suggest past interaction. The overall morphology suggests a relatively evolved system with a moderately low star formation rate.
