The galaxy presents as a roughly elliptical structure, with a smooth appearance and no readily discernible spiral arms or bar features. The central region appears as a bright, concentrated bulge, suggestive of a high stellar density. The color gradient transitions from a yellowish-white core to a bluer periphery. The overall morphology indicates a likely classification as an elliptical or lenticular galaxy. There is a slight indication of a flattened shape, leaning towards an in-between roundedness classification. No major disturbances or signs of ongoing merging activity are immediately apparent in the image; however, a slight asymmetry exists which could be from a minor disturbance. The galaxy appears relatively undisturbed.
