The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, the brightest and most prominent region in the image, with a color leaning towards yellow-orange. This suggests an older stellar population dominating the core.

The light from the core dissipates outwards, with a more diffuse halo surrounding it. A slight flattening is observed, indicative of a shape deviating from perfect sphericity. There is little indication of any prominent spiral arm structure or significant dust lanes within the galaxy. The outer regions appear relatively featureless, showing a gradual fading into the background sky. Some minor colour variation is seen in the surrounding halo, with hints of slightly bluer regions mixed amongst the warmer colours. There is no obvious indication of a major ongoing merger, however the overall shape hints that it may have had minor disturbances.
