The galaxy presents as a primarily smooth and concentrated elliptical or lenticular morphology. It appears relatively featureless, lacking prominent spiral arms or a distinct disk structure. The light is concentrated towards the center of the galaxy, suggesting a well-defined core or bulge component. A slight elongation is barely noticeable, and it seems to be more "in between" round and cigar shaped. There are no clear signs of any major ongoing merger events. It appears to be a static galaxy, though possibly experiencing minor disturbances. Based on its apparent color gradient, it seems to have redder hues in the central core.
