The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The color gradient transitions from a bright, yellowish core region to a bluer, more diffuse outer halo. The core exhibits a high degree of symmetry, indicative of an older stellar population dominating its luminosity. There is minimal evidence of significant star formation activity within the visible light spectrum. The galaxy shows no clear signs of spiral arms or significant dust lanes and has an intermediate roundness, appearing more disc-like than spherical. There are slight asymmetrical extensions or minor distortions in the halo, which might indicate recent interaction. However, no major tidal features or other clear indications of a major merger event are readily apparent.
