The galaxy presents as a luminous, centrally concentrated object with a smooth overall appearance. It exhibits a generally elliptical morphology, with a high degree of roundness and a slight yellow-orange hue, potentially indicative of an older stellar population. There is a hint of some possible disturbances in the morphology. The galaxy does not appear to have any readily identifiable spiral arm structure or a prominent disk-like component. Its integrated color suggests moderate star formation. The system seems to be in the process of a major merging event.
