The galaxy presents as a centrally concentrated, elliptical morphology with a smooth light profile. The core exhibits a yellowish-white hue, suggesting an older stellar population, indicative of diminished star formation. The galaxy's isophotes appear relatively round, though there may be a slight elongation along one axis. There are no readily apparent signs of spiral arms, dust lanes, or active galactic nuclei activity. The outer regions of the galaxy fade gradually into the background, hinting at a diffuse halo. There is little evidence of recent or ongoing merger activity or significant tidal disturbances.