The galaxy presents a morphology suggestive of a system undergoing a merger. There appears to be two distinct nuclei, one exhibiting a redder hue and the other appearing more yellowish-white. Extended, but somewhat irregular, diffuse emission surrounds these nuclei. The overall shape is not distinctly elliptical or spiral, lending support to the interaction classification. The galaxy exhibits a moderate size. The color gradients suggest variations in stellar populations or dust content across the object. There may be some disturbances present.
