The galaxy appears to be a relatively compact, elliptical type. Its light profile suggests a smooth, centrally concentrated morphology with a high degree of symmetry. Color gradients are subtle, with a slightly redder core region transitioning to a bluer halo, potentially indicating a difference in stellar populations. There is very little to no visual evidence of a disk or spiral arms. No strong tidal features or obvious signs of recent mergers are apparent. The galaxy shows no strong dust lanes or patchiness within the image.