The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a near-circular morphology. There is a bright central region that appears to be the nucleus. The color of the nucleus trends towards yellow-white. The outer regions show a subtle color gradient shifting towards blue-green, suggesting the presence of a younger stellar population in these regions. The light is relatively uniform, lacking strong evidence of spiral arms or significant dust lanes. The galaxy does not appear to be undergoing any major mergers, and displays minimal signs of tidal disturbances.