The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. Moving outwards, the galaxy gradually fades into a more diffuse halo, exhibiting a bluer tint which could point to the presence of younger stars, though the rate of star formation is probably quite low. There is no apparent spiral structure or significant dust lanes visible in this image, reinforcing its classification as an elliptical galaxy. No obvious signs of tidal disturbances or ongoing mergers are observed, implying the galaxy is relatively undisturbed. The shape is close to circular, deviating only slightly.
