The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. There is evidence of a more diffuse, bluer halo extending outwards from the central region, which might indicate ongoing or recent star formation activity within the galaxy's outer regions, though at a low rate. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions based on its shape. The overall color profile suggests a population of both older stars in the core and a small amount of younger stars distributed throughout the surrounding halo.
