This galaxy presents as an elliptical-type galaxy, displaying a largely smooth morphology without prominent spiral arms or a significant disk structure. The galaxy exhibits a centrally concentrated bulge, appearing brighter and more compact in the center.

The color gradient suggests a redder hue in the central regions, possibly indicative of an older stellar population. The outer regions appear marginally bluer, which may reflect the presence of younger stars, albeit to a much lesser extent than what would be observed in a typical spiral galaxy. Overall, the galaxy appears relatively undisturbed, without strong evidence of ongoing major mergers or tidal interactions. There is a slight elongation that may suggest it is not perfectly spherical.
