This galaxy presents as a relatively smooth, centrally concentrated object. Its morphology suggests an elliptical or lenticular classification, lacking prominent spiral arms or distinct features indicative of active star formation regions within a disk. The galaxy exhibits a high degree of central symmetry, and the outer regions of the galaxy gradually fade into the background. The color profile appears to be dominated by yellowish hues, suggesting a population of older stars. There is no evidence of any major disturbances or ongoing mergers, with no significant tidal tails or asymmetries visible. Overall, this galaxy appears to be a passively evolving system.
