The galaxy appears to be elliptical in shape, displaying a smooth, featureless morphology. The light distribution is concentrated towards the center, with a gradual decrease in luminosity towards the edges. There is a slight elongation observed, and its overall appearance suggests it is in a relatively quiescent state. Possible minor disturbances may be present within the galaxy's halo. The color profile indicates a relatively uniform stellar population, consistent with an older population of stars.
