The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The core region exhibits a bright, yellow-white hue, suggesting a population of older stars. Surrounding the core, a bluer, diffuse halo extends outwards, indicating the presence of some younger stars or ongoing star formation at the periphery. The overall structure appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. There is a slight elongation along one axis, deviating somewhat from a perfect circular shape, which might be indicative of a mild interaction or internal dynamics. The galaxy appears to be a relatively massive system.
