The galaxy appears to be a luminous, relatively smooth and centrally concentrated object. It exhibits a generally elliptical morphology, close to round, with a significant central bulge. The light profile suggests a centrally dominant stellar population, with a color gradient indicative of older stars dominating the core. There is little evidence of prominent spiral arms or distinct features. The galaxy appears to be relatively undisturbed, lacking signs of major mergers or strong tidal interactions. There are no obvious indications of ongoing, vigorous star formation regions.
