The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge with a gradual decrease in luminosity outward. The galaxy displays a yellowish-white hue, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes. The overall structure is largely undisturbed, indicating that the galaxy has likely not undergone a major merging event recently, although some minor disturbance cannot be ruled out. The shape is generally round. The estimated size suggests that it is a massive galaxy, with a low rate of star formation.
