The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated light profile, with a gradual decrease in luminosity moving outwards from the core. The core region appears yellowish, potentially indicating an older stellar population. There is little evidence of spiral arms or significant dust lanes. The galaxy appears mostly undisturbed, with no obvious signs of major mergers or tidal interactions. The morphology suggests a relatively evolved system that may have exhausted much of its gas supply for star formation.
