The galaxy presents as an elliptical morphology, displaying a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish-white hue, suggesting an older stellar population. The isophotes appear relatively undisturbed, showing a slight elongation but minimal signs of significant tidal interactions or recent mergers. Faint bluish-white fringes extend outwards from the central region, possibly indicating a small amount of younger star formation in the outer regions of the galaxy. The overall structure gives the impression of a mature galaxy with little current star formation.
