The galaxy presents as a diffuse, centrally concentrated object exhibiting a non-uniform distribution of light. There appear to be two main concentrations of light. The upper, larger area is bluer, while the lower is redder. The blue is concentrated in the center of that section. The red section also has more light concentrated in its center. The overall morphology suggests a system undergoing a merger or significant interaction, potentially between two distinct galaxies or a single galaxy with a large, disruptive companion. The object is not perfectly smooth; some disturbances in the overall structure are apparent. The object does not appear to be a late-stage merger, but rather at a point where individual objects are still somewhat discernible, though greatly distorted.
