The galaxy presents as a relatively smooth, centrally concentrated structure, likely an elliptical or S0 type. There is an absence of distinct spiral arms or prominent dust lanes. The light distribution is generally diffuse, fading gradually from the bright central region outwards. The shape is roughly elliptical, with a moderate degree of ellipticity, leaning towards round. There is no obvious evidence of ongoing major mergers or strong tidal disturbances in its immediate vicinity, although some minor asymmetry cannot be ruled out. The color is generally redder, which would imply a population of older stars and a lack of significant recent star formation. Overall, it appears to be a massive galaxy with a well-established stellar population.
