The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge, with a gradual decrease in luminosity outwards. The light profile suggests an evolved stellar population, with a yellowish-red hue dominating the core region. There is little evidence of significant dust lanes or prominent spiral arm structures. The galaxy appears relatively undisturbed, lacking obvious signs of recent major mergers or tidal interactions. Overall, the galaxy appears to be a quiescent elliptical galaxy with a significant population of older stars.
