The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular system. It displays a slightly elongated morphology, approximating a flattened spheroid. A bright, diffuse central bulge dominates the galaxy's light profile, with a gradual fading outwards towards its periphery. There is little indication of resolved spiral arms or significant dust lanes. Faint hints of an extended halo region are discernible surrounding the main body of the galaxy, though this is very diffuse. The light from the galaxy appears slightly red-shifted. No evidence of ongoing major mergers or significant tidal disturbances are apparent in the visible light.
