The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge that diffuses outwards. The color profile suggests a mixed population of stars. The core shows a concentration of older, redder stars, while the outer regions appear slightly bluer, possibly indicative of younger stellar populations. The overall form appears largely undisturbed, with no obvious signs of ongoing major mergers or tidal disruptions. There's a subtle suggestion of a flattened shape, trending towards a more disk-like structure, but it maintains a predominately spheroidal appearance. The galaxy's star-forming activity appears subdued, with a dominance of evolved stellar populations. Overall, the galaxy likely represents a mature system undergoing gradual evolution.
