The galaxy presents as a smooth, centrally concentrated elliptical structure with a high degree of circular symmetry. The light profile is highly concentrated, with a bright, well-defined core transitioning to a fainter, diffuse outer region. No prominent spiral arms or disk features are discernible within the image resolution. The galaxy's color appears generally red, indicating an older stellar population, though there are hints of a slight bluer hue in the outer regions. No obvious signs of tidal interactions or recent mergers are visible.
