The galaxy presents as a centrally concentrated object with a bright, unresolved core. Surrounding the core is an extended, diffuse halo exhibiting a degree of granularity, suggesting a composite stellar population. The overall color is broadly consistent with a relatively mature stellar population, with a moderate contribution from younger stars. The morphology appears to be primarily spheroidal, though there is faint evidence of a possible disk component. There also appears to be some potential minor disturbances visible near the edges of the disk. There is no indication of a strong tidal interaction or recent major merger. Overall the galaxy appears to be relatively undisturbed.
