The galaxy presents as a relatively bright, centrally concentrated system. Its overall morphology appears to be that of an elliptical or lenticular galaxy, with a smooth, diffuse light distribution. The central bulge is prominent, exhibiting a high degree of luminosity. There is a hint of a disk-like structure extending outwards from the bulge, but it is not clearly defined, and is relatively featureless. Some disturbances are noticeable, but not exceptionally large. The galaxy exhibits a subtle blue tinge in the outer regions, suggesting some ongoing, though possibly low-level, star formation. There is no significant spiral arm structure visible. The galaxy appears to be in the process of, or having recently undergone, a merger event, with one side more disturbed than the other.
