The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse light distribution. There is little evidence of spiral arms or other distinct morphological features beyond the central bulge. The galaxy exhibits a color gradient, appearing more yellow-reddish toward the core and gradually becoming bluer in the outer regions. This suggests an older stellar population is dominant in the central regions. The object appears fairly undisturbed, with no obvious signs of recent major mergers or tidal interactions. Faint extensions or halos may be present, but their low surface brightness makes it difficult to ascertain their nature and extent from this image alone.
