The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, featureless morphology with no discernible spiral arms or a prominent central bulge. The galaxy appears to be mostly round, with minimal elongation. The light distribution is centrally concentrated, fading gradually towards the outer edges. There are no indications of any major mergers or strong tidal disturbances, although there is a chance for minor disturbances to be present. Based on the overall color, the stellar population is likely dominated by older stars, with a low star formation rate. The galaxy appears to be a quiescent system, with little evidence of ongoing star formation.
