The galaxy presents as a centrally concentrated object with a generally elliptical morphology. There is a smooth, extended halo surrounding a bright, condensed core region that is yellowish in hue. The isophotes appear relatively regular, suggesting a relaxed system without significant ongoing mergers. The colour gradient from the core outwards suggests potential variations in stellar populations, with the central regions possibly exhibiting a higher fraction of older, redder stars. There is no obvious spiral arm structure or strong dust lane present, consistent with the interpretation of a spheroidal galaxy. Faint tidal features or subtle perturbations are possibly present, though not readily discernible given the image resolution.
