This galaxy presents as a largely featureless elliptical. It has a generally smooth appearance, with a high degree of central concentration. The core exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the galaxy transitions to a more diffuse halo. The halo exhibits a bluer tint compared to the core, suggestive of ongoing or recent star formation, although at a relatively low rate. The isophotes appear mostly circular and regular, with only minimal evidence of tidal disturbances or interactions. The overall morphology indicates a relatively evolved system, likely a massive galaxy that has undergone significant merging or accretion in its past, resulting in its present smooth and rounded appearance.
