This galaxy exhibits a complex morphology, suggestive of an ongoing or recent interaction with a nearby galaxy. At least two distinct luminous components are visible, one appearing more spheroidal and the other being more disk-like, viewed close to edge-on. The spheroidal component displays a smoother light distribution and a yellowish tint. The disk-like component has a distinct bulge. The galaxy system is relatively compact, with a significant amount of interaction in the core. The system displays a blue tint in the innermost regions which may suggest ongoing star formation. The overall structure is irregular, indicating gravitational disturbance possibly due to a merger event. 
