The galaxy appears to be a relatively smooth, elliptical galaxy at a moderate redshift. It exhibits a centrally concentrated bulge with a diffuse halo extending outwards. There is little indication of prominent spiral arms or significant dust lanes. The galaxy's shape is somewhat rounded, with a subtle elongation. The color profile suggests a population of older stars dominating the central region, inferred from the reddish hue, with a slightly bluer color in the outer regions, potentially indicating some ongoing, albeit low-level, star formation. There is no obvious evidence of major mergers or significant tidal disturbances.
