The galaxy presents as a centrally concentrated, elliptical system. The core exhibits a bright, yellowish-white hue, suggesting a substantial population of older stars. The galaxy appears relatively smooth in texture, with a gradual decrease in luminosity moving outwards from the center. The overall shape appears somewhat rounded. There is a slight suggestion of a disk component. No prominent spiral arms or dust lanes are discernible. Based on the color, the star formation rate is likely low.
