The galaxy presents as a relatively smooth, elliptical-like structure with a somewhat rounded appearance. It displays a bright, concentrated central region, potentially indicating an active galactic nucleus or a dense stellar population. Faint extensions or diffuse halos may surround the core, though this is difficult to ascertain with certainty. The color profile suggests a composition of older stellar populations, as evidenced by the redder hues, although there is some slight green tint. Overall, it does not appear to be undergoing any major mergers or significant tidal disruptions, with the structure appearing relatively quiescent.