The galaxy presents as a relatively smooth, elliptical morphology. It appears largely spheroidal in shape with a high degree of radial symmetry. There is no discernible disk structure, spiral arms, or bar. The light distribution is concentrated toward the center, and fades gradually outward. Its color appears yellow-orange, indicative of a dominant population of older stars. No signs of active star formation regions or dust lanes are visible in the galaxy. Based on the undisturbed morphology, the galaxy does not show evidence of recent major mergers.
