The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The light diffuses outward from the center in a smooth gradient, transitioning to a redder tone. There are no visible spiral arms or dust lanes. The galaxy appears relatively undisturbed, with a high degree of radial symmetry. It lacks any obvious signs of ongoing star formation, presenting a generally quiescent appearance.
