The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge which transitions into a more diffuse halo. The overall color is somewhat redder in the core, suggesting an older stellar population, with a gradual shift towards bluer hues in the outer regions, possibly indicating ongoing or recent star formation at a low rate. There are some minor, subtle disturbances in the outer regions, indicating the possibility of a past interaction. The galaxy has a generally round shape.
