The galaxy appears as a singular, concentrated light source. It exhibits a predominantly smooth morphology with a largely featureless structure. The light is primarily yellowish-white, which may indicate an older stellar population. The shape is generally round, displaying only a slight deviation from perfect circularity. There is no distinct indication of spiral arms or a prominent disk. Faint hints of a nebulous extension surround the bright core, suggesting a diffuse halo component. No signs of major ongoing mergers or strong tidal distortions are observed; any irregularities are minimal. The galaxy appears as an elliptical galaxy type.
