The galaxy presents as a slightly elongated, elliptical morphology. Its central region exhibits a high surface brightness, appearing yellowish-white, indicative of a population of older stars. The galaxy's light gradually fades towards its outer edges, showing a smooth transition without prominent spiral arms or distinct features. The color gradient suggests a radial change in stellar populations, possibly with younger, bluer stars more prevalent in the outer regions, although this is not as apparent as in spiral galaxies. The overall structure appears relatively undisturbed, showing no signs of major mergers or tidal interactions, though a slight asymmetry cannot be ruled out.
