The galaxy presents as a generally smooth, elliptical-like structure. There is a distinct, bright central bulge exhibiting a yellowish-white hue, suggesting an older stellar population. This brighter, more concentrated region gradually fades into a more diffuse halo. The outer regions of the galaxy display a slightly reddish tint. The galaxy's shape deviates somewhat from perfectly circular, appearing slightly elongated. There are no readily discernible spiral arms or prominent dust lanes. No obvious signs of interaction or major disturbances are observed. Overall, the galaxy appears to be a relatively quiescent system.
