The galaxy appears as a single, concentrated source of light, roughly elliptical in shape. The light is yellowish-white, indicating a population of older stars. The galaxy is smooth and has a high degree of central concentration. There is no strong evidence of spiral arm structure or a prominent disk. There is a possibility of a minor gravitational disturbance or tidal feature. The galaxy is not undergoing an active major merger event. The observed properties are consistent with an early-type galaxy or elliptical galaxy.
