The galaxy presents as a largely featureless, elliptical morphology. Its light profile is concentrated towards the center, with a smooth, gradual decrease in luminosity moving outward. The central region exhibits a bright, unresolved core, likely indicative of a galactic nucleus. There is a subtle color gradient, with the core exhibiting a slightly yellower or redder hue compared to the outer regions of the galaxy, suggesting a population of older stars concentrated in the center. No prominent spiral arms, dust lanes, or star-forming regions are discernible. The galaxy appears relatively undisturbed, showing no signs of recent mergers or tidal interactions. It presents a largely symmetrical structure.
