The object appears to be a galaxy, likely an elliptical or lenticular type. It presents a generally smooth morphology. There is some indication of a flattened disk-like structure, viewed nearly edge-on, with a brighter central bulge. The galaxy's color suggests an older stellar population dominating its composition. There may be some dust rings. There are no strong indicators of recent or ongoing major mergers, though subtle disturbances cannot be ruled out entirely. The overall structure exhibits a moderate degree of roundness, being neither perfectly spherical nor excessively elongated.
