The galaxy presents as a centrally concentrated object, with a smooth, elliptical morphology. The color appears to be a yellow-white hue, suggestive of an older stellar population with minimal ongoing star formation. There is little evidence of spiral arms or a distinct disk structure. The galaxy's light profile decreases smoothly and gradually outwards from the center. No obvious tidal features or signs of recent mergers are apparent upon visual inspection. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
