The object appears to be a galaxy, likely an elliptical type based on its overall morphology. It exhibits a smooth, centrally concentrated light distribution with a notable lack of spiral arm structures or prominent dust lanes. The galaxy presents as elongated, more cigar shaped than round, suggesting a possible E4-E7 classification on the Hubble sequence. There's a bright, unresolved core, implying a high stellar density or possible active galactic nucleus (AGN), however, based on the color, that is unlikely. The overall color index suggests a population of older stars, with minimal ongoing star formation. There appears to be no major interaction or disturbance in this galaxy.
