The galaxy presents as a relatively compact object, exhibiting a somewhat disturbed morphology. The primary structure appears to be composed of two distinct luminous components. The system is generally elliptical in shape, though this is disrupted by potential tidal features. There is a smooth gradient of light that surrounds the two luminous cores. The colour profile suggests ongoing star formation, indicated by a blue tinge, but the overall red colour suggests a more evolved stellar population as well. There is possible evidence of merging or recent interaction, given the asymmetry and the dual-core appearance. A faint plume or tail-like structure may be present.
