The galaxy presents an overall smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region residing in the core. There is a subtle elongation observed, suggesting a deviation from a perfect spherical shape. The color gradient indicates a somewhat bluer core region, possibly indicative of younger stellar populations or ongoing star formation, while the outer regions appear redder, potentially representing older stellar populations. There is no apparent evidence of strong spiral arm structures or significant dust lanes. The morphology appears largely undisturbed, with no major signs of mergers or tidal interactions. The observed size suggests this is a galaxy of moderate physical extent.
