The galaxy presents a generally smooth, elliptical morphology. There is a high degree of central concentration. Its overall color appears to be a pale blue, indicating the presence of some younger, hotter stellar populations, but the dominant light seems to be in the redder portions of the visible spectrum. There is no obvious presence of spiral arms or a prominent galactic disk. No active galactic nucleus is visible, and there are no signs of any ongoing major mergers or significant tidal distortions. The galaxy appears quite isolated.