The galaxy presents as a relatively smooth, elliptical-shaped object. It exhibits a concentrated central bulge with a yellow-orange hue, indicating a population of older stars. There is a faint, diffuse halo surrounding the core, suggesting the presence of a stellar envelope extending beyond the main body. The galaxy appears to be relatively isolated, with no obvious signs of major interaction or ongoing merger activity, though a minor disturbance cannot be ruled out. Overall, the galaxy appears to be a mature, relatively quiescent system.
