The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated light profile, with a gradual decrease in luminosity extending outwards. The core appears bright and yellowish, possibly indicating an older stellar population. No distinct spiral arm features or significant dust lanes are discernible in the available image. The galaxy appears largely undisturbed, lacking any obvious signs of major mergers or tidal interactions, though there may be a minor disturbance. The general morphology suggests a spheroid-dominated galaxy.
