The galaxy exhibits a morphology suggestive of a potentially disrupted system. It displays a diffuse, centrally concentrated structure, but lacks the distinct features of a well-defined spiral or elliptical galaxy. There is some indication of minor asymmetry in the light distribution, suggesting a possible interaction or disturbance. Redder light is seen to dominate the central region of the galaxy. The galaxy is relatively small in apparent size. There are some features that could be either artifacts or represent potential merging components.
