This galaxy appears to be a relatively large elliptical galaxy at a considerable distance. Its morphology is dominated by a smooth, centrally concentrated distribution of light, suggesting an older stellar population. The overall color is yellowish, which is consistent with an evolved stellar population, depleted of young, blue stars. There is no evidence of spiral arms or a prominent disk structure. The light distribution is fairly symmetrical and generally round in shape, with no obvious signs of significant tidal disturbances or ongoing mergers. The presence of some irregularities in the light distribution may indicate previous minor interactions or internal activity, but the overall impression is one of a relaxed, passively evolving system.
