The galaxy presents as a relatively smooth, elliptical structure. It has a dominant central bulge that appears nearly spherical. The light profile suggests minimal star formation. There is a concentration of older stars within the central regions. The galaxy exhibits a color gradient, with the central region appearing slightly redder than the outer regions, suggestive of an aging stellar population. There is a noticeable lack of spiral arms or significant dust lanes. The galaxy appears isolated, with no obvious signs of tidal interactions or ongoing mergers, and the outer regions are not well-defined.
