The galaxy presents as a single, relatively smooth object with a concentrated central bulge. It exhibits a primarily yellow-orange hue, suggesting a stellar population dominated by older stars. There are no discernable spiral arms or distinct features associated with active star formation. The morphology appears generally elliptical or spheroidal, lacking a prominent disk structure. There is no evidence of tidal tails or distortions that would indicate a recent or ongoing merger event, although a minor disturbance cannot be completely ruled out. The overall light distribution is centrally concentrated, and its estimated size is close to 6 kpc. Given its color and morphology, this galaxy is likely a passively evolving system with a low specific star formation rate.
