The galaxy presents as an elliptical morphology, appearing largely featureless and smooth in texture. Its light is centrally concentrated, displaying a bright, relatively uniform core region that graduates into a diffuse halo. The observed color suggests an evolved stellar population, trending towards redder wavelengths. There is minimal evidence of spiral arms or active star formation regions visible within the galactic structure. The overall shape appears roughly circular. There is no obvious indication of ongoing major mergers or tidal disturbances. However, there are very faint signs of some possible minor disturbances that could possibly be the remnants of a past merger.
