The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable color gradient, shifting from a bluer hue at the outer edges to a yellower, redder hue towards the core. This could indicate a difference in stellar populations, with older, redder stars dominating the central region and younger, bluer stars residing in the outer regions. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent mergers, though there is a slight elongation. The absence of prominent dust lanes or spiral arm structures suggests it is likely an early-type galaxy with a relatively low rate of current star formation.
