The galaxy appears to be a relatively smooth, elliptical system. It presents a concentrated central bulge that gradually fades into a more diffuse halo. The light profile suggests a high degree of sphericity, with minimal visible disk-like features or spiral arm structures. Color gradients across the galaxy are subtle but visible. The core exhibits a slightly yellower hue, while the outer regions display a bluer tint. The lack of significant dust lanes or prominent star-forming regions reinforces the impression of a morphologically evolved system. There are no strong signs of tidal disturbances or ongoing merger activity.
