The galaxy presents as a somewhat smooth, elliptical-like object, with a concentrated central bulge. The overall color appears to be slightly reddish-yellow, suggesting a population of older stars, potentially indicating reduced star formation activity, or possibly dust obscuration. There are no obvious spiral arms or distinct disk-like features visible in this image. The galaxy appears relatively isolated, with no immediately apparent signs of tidal disturbances or ongoing merger activity. The light is primarily concentrated in the core, fading gradually outward, displaying a fuzzy, diffuse halo.
