The galaxy appears as a relatively smooth, centrally concentrated object. There is little to no discernible disk structure or spiral arms. The light distribution exhibits a high degree of radial symmetry, with an apparent ellipticity close to circular. The central region is brighter and exhibits a yellowish color, suggesting a population of older stars. The outer regions are dimmer and somewhat bluer, indicating the presence of some younger stars, although the overall color suggests this galaxy is redder and more evolved. There is no evidence of any major ongoing merger activity or strong tidal features; it appears to be an undisturbed system. The object's smooth morphology and color profile suggest it is a relatively early-type galaxy.
