This galaxy exhibits a relatively smooth morphology, indicative of an elliptical or lenticular type. It appears centrally concentrated with a bright, unresolved nucleus. The galaxy's overall shape is generally round, with minimal deviation from circular symmetry. There's a faint, diffuse halo extending outwards from the central region. No distinct spiral arms or prominent dust lanes are discernible. The color gradient suggests a population dominated by older stars, with a redder hue in the outer regions, and a slight brightening, more blue core. No obvious signs of major ongoing mergers or tidal disturbances are visible. The low star formation rate suggests that this galaxy has largely exhausted its supply of gas for star formation. Some minor disturbances are faintly visible, though no major merger is evident.
