The galaxy presents as a relatively smooth, centrally concentrated object. There is evidence of a faint, diffuse halo extending outwards from a brighter core region. The overall shape appears roughly elliptical, with the ratio of the minor to major axis suggesting a moderate degree of flattening. The galaxy exhibits a color gradient, with the central region appearing yellower compared to the bluer, more diffuse outer regions. There is no distinct spiral arm structure or prominent dust lanes visible. The galaxy appears largely undisturbed, with no major signs of ongoing mergers or tidal interactions. Based on its morphology, it is likely an early-type galaxy, with a significant population of older stars dominating its stellar content.
