The galaxy presents as a relatively smooth, elliptical-like structure with a distinct central bulge. The core region exhibits a yellowish-white hue, potentially indicating an older stellar population. A diffuse, bluer halo surrounds the central region, suggesting the presence of some younger, hotter stars, though this appears to be minor. The overall shape is somewhat elongated rather than perfectly spherical, with no discernible spiral arm structure. There are hints of minor irregularities or disturbances in the outer regions, though no major mergers or tidal features are readily apparent.
