The galaxy presents as a single, relatively smooth object with a centrally concentrated luminosity profile. The core exhibits a yellow-white hue, suggesting a population of older stars. Moving outward from the center, the color transitions to a more subdued yellow-orange, with a diffuse halo. The morphology appears to be elliptical. The galaxy shows no evidence of spiral arms or significant dust lanes, but a slight elongation is visible. There is no clear indication of tidal features or ongoing major merger activity, though minor asymmetries or disturbances cannot be ruled out based on this image alone. Overall, the galaxy appears to be a mature system with a high degree of symmetry and little to no evidence of active star formation.
