The galaxy presents a generally elliptical morphology. The light profile appears smooth and centrally concentrated, showing a gradual decrease in luminosity outward from the core. The central region exhibits a reddish hue, potentially indicating an older stellar population and/or dust obscuration. Surrounding the core, there is a more diffuse yellowish-white halo, which could be indicative of a younger stellar population compared to the core or simply due to a different ratio of stellar types. There is no indication of spiral arms or a distinct disk structure, and it appears to be relatively undisturbed, without strong signs of recent mergers or tidal interactions. The galaxy appears to be a relatively massive and evolved system.
