The galaxy presents as a spheroid with a smooth, relatively featureless morphology. The light profile appears concentrated towards the center, suggesting a prominent bulge. Color gradients indicate a relatively older stellar population, particularly in the central region where the light is redder. There is a slight asymmetry to the galaxy's shape, with a small extension visible on one side, but there is no clear indication of a major ongoing merger or tidal disturbance. Overall, it appears to be a relatively quiescent galaxy.
