The galaxy appears as a relatively compact, elliptical system with a smooth, diffuse light profile. There is a bright central core, surrounded by a more extended, fainter halo of light. The overall shape is generally round. There is no evidence of distinct spiral arms, bars, or a well-defined disk structure. The galaxy exhibits a subtle color gradient, appearing slightly bluer in the outer regions compared to the core, suggesting some degree of ongoing or recent star formation, although the dominant stellar population likely consists of older stars. No signs of major mergers or tidal disturbances are immediately apparent; the galaxy seems isolated and undisturbed.
