The galaxy presents as a diffuse, elliptical-like structure with a bright, concentrated central bulge. There is a noticeable fall-off in luminosity from the core outwards, but no sharp edges, with a smooth transition into the background sky. The galaxy appears generally featureless. Color gradients indicate potentially older stellar populations. There is a suggestion of a slight disk-like structure surrounding the central bulge. No clear spiral arm structure, dust lanes, or active star-forming regions are discernible. The galaxy's shape appears generally undisturbed, without any obvious signs of tidal interactions or mergers.
