The galaxy appears as a yellowish, centrally concentrated object. It exhibits a relatively smooth light distribution, lacking prominent spiral arms or distinct features typically associated with disk galaxies. The morphology suggests a spheroidal shape, leaning towards a round appearance. There's no obvious visual evidence of ongoing major mergers or significant tidal disturbances in its immediate vicinity. The galaxy's color index suggests a population of older stars with a relatively low rate of current star formation. Considering these factors, it's likely a massive, evolved galaxy.
