The galaxy presents as a single, centrally condensed object. The central region exhibits a bright, yellowish-white hue, suggesting a dominant population of older stars. The overall shape appears to be elliptical, though with slight elongation that may indicate it is not perfectly spherical. There is little discernible spiral structure. 

There appears to be an extended halo of fainter material surrounding the central concentration. The outer regions show a slightly bluer tint compared to the core, which could be indicative of younger stars within the extended halo or simply an artifact.

Based on the smooth appearance of the galaxy and the lack of any tidal features or other disturbances, it appears to be a relatively undisturbed system. There is no obvious evidence of recent or ongoing mergers or interactions with other galaxies.
