The galaxy presents as a centrally concentrated, ellipsoidal structure with a smooth light distribution. The core exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. There is a slight elongation to the galaxy's shape, hinting at a possible prolate spheroid morphology rather than a perfectly spherical one. A faint, diffuse halo surrounds the central region, appearing greenish in color, possibly indicating the presence of some younger stars or ongoing, low-level star formation activity. There is no apparent evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no clear signs of a recent major merger event. Overall, it appears to be a massive, early-type galaxy with a moderate redshift.
