The galaxy presents a primarily smooth morphology, with a concentrated central bulge. There is a slight extension beyond the central region, indicating a possible disk-like structure, though it appears relatively faint and unstructured. Color gradients suggest the presence of older stellar populations, with reddish hues dominating the outer regions. There is no readily apparent active galactic nucleus or distinct dust lanes. The overall structure appears mostly undisturbed, with no major signs of ongoing or recent mergers. A small amount of asymmetry can be seen, possibly from a minor disturbance. The system appears more elliptical than spiral in nature.