The galaxy appears to be a relatively small, elliptical galaxy, classified as mostly smooth, with a slight elongation. It is largely featureless, lacking any distinct spiral arm structure or prominent dust lanes. The galaxy exhibits a centrally concentrated bright region with a diffuse halo extending outwards. The color profile suggests a population of older stars, indicated by the reddish hue in the outer regions, contrasted by a bluer core, potentially indicative of some ongoing star formation. There is no evidence of a major merger or significant tidal disruption, although subtle irregularities might suggest a minor interaction or disturbance. Overall, it appears as a relatively isolated and evolved system.
