The galaxy presents as a largely smooth, elliptical structure. Its overall shape is substantially round. The core exhibits a concentrated, bright yellowish-white luminosity, suggesting a high density of older stellar populations. The outer regions display a more diffuse, reddish-tinged halo. There is little evidence of spiral arms or distinct features in the image, pointing towards a more evolved morphology. The galaxy appears relatively undisturbed, with no obvious signs of ongoing mergers or major interactions. The overall color suggests a population of older stars and a low rate of current star formation.
