The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. It appears elliptical in shape, with a higher intensity core that gradually fades into a less defined outer region. The color profile is relatively uniform, with a noticeable orange-red hue, suggesting an older stellar population. There is no clear indication of spiral arms, a disk structure, or significant dust lanes. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions, though a slight asymmetry cannot be ruled out.
