This galaxy appears to be a relatively smooth, elliptical system. The light is concentrated towards the center, with a gradual decrease in surface brightness moving outwards. The galaxy has a generally round shape, with a smooth appearance and no obvious spiral arm structures or bars. The core shows a yellowish-orange hue, likely indicating an older stellar population. The outer regions appear somewhat bluer in comparison, which may suggest the presence of a younger population of stars, even if the overall star formation rate is relatively low. There is no evidence of major mergers or significant tidal disturbances in its immediate vicinity, with no apparent close companions or streams.
