The galaxy presents an elliptical morphology. Its central region exhibits a high surface brightness, appearing nearly spherical with a smooth, concentrated distribution of light. Moving outward, the galaxy gradually fades into a more diffuse halo. There is no visible dust lane or spiral arm structure, which supports its classification as an elliptical galaxy. There are no signs of strong tidal interactions or major mergers, but there could be some tidal distortion or minor disturbance. Overall, the galaxy appears to be relatively undisturbed. The color profile suggests a population of older stars, with the central bulge leaning toward yellow.
