The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears to be largely spheroidal, with minimal discernible disk-like features. The light profile exhibits a centrally peaked core, surrounded by a more diffuse halo. There is some evidence of bluer emission extending from the central region, potentially indicating areas of recent or ongoing star formation, although this activity appears subdued. Overall, the galaxy gives the impression of an evolved system with primarily older stellar populations dominating its luminosity. There are no indications of major mergers or significant tidal disturbances.
