The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. Its core exhibits a yellowish-white hue, indicative of an older stellar population. The galaxy fades outward from the center with a noticeable decrease in brightness. Moving outwards, a blueish cast indicates pockets of younger star formations are likely present. The galaxy lacks any obvious spiral arm structure or distinct features, suggesting an elliptical or lenticular classification. Its apparent roundness supports this hypothesis. There are no obvious signs of recent or ongoing major mergers, though there is a slight asymmetry that could indicate a minor gravitational interaction in the past. The overall structure appears relatively undisturbed.
