The galaxy appears as a single, elliptical-like object. The light profile is smooth and centrally concentrated, with a lack of discernible spiral arms or disk features. The overall color of the galaxy is strongly indicative of a redder population of stars. There is no evidence of significant dust lanes or patches. The galaxy exhibits a fairly regular morphology, with a high degree of roundness. There are no obvious signs of tidal tails or other significant gravitational disturbances that would indicate a recent major merger event, although a possible minor interaction cannot be ruled out.
