The galaxy presents as a centrally concentrated, relatively smooth system. Its overall morphology appears elliptical, with a high degree of radial symmetry. A bright, somewhat diffuse nucleus is apparent, indicating a concentration of stars towards the center. The galaxy appears to be yellowish-orange in color, which suggests an older stellar population. There is little evidence of spiral arms or active star formation. The outskirts of the galaxy gradually fade into the background, without any sharp edges or tidal features. There are no visible signs of ongoing major mergers or significant disturbances. A faint disk may be present but is difficult to resolve.