The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-white, suggesting a population of older stars. Surrounding this central region is a fainter, more diffuse halo with a slight greenish hue. There are no obvious spiral arm structures or dust lanes visible in this image, lending credence to the smooth classification. The galaxy appears relatively undisturbed with no apparent signs of ongoing or recent mergers.
