The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that graduates into a diffuse halo. The galaxy's color profile suggests a population of older stars, with a redder hue throughout the galaxy, with faint yellow tinge towards the center. There are no discernible spiral arms or dust lanes. The galaxy appears relatively undisturbed, showing no significant signs of tidal interactions or recent merger activity. It presents as an isolated, evolved system.
