The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a yellowish-white hue, indicative of a dominant population of older stars. Moving outward from the center, the color appears to shift slightly toward a redder tone. The galaxy's overall structure is largely smooth with no apparent signs of spiral arms or significant dust lanes, indicative of a more evolved system. The halo appears faint, lacking distinct features and merging smoothly with the background sky. There is no visible evidence of a major ongoing merger or tidal interactions.
