The galaxy appears to be undergoing a merger or interaction. One component presents a relatively smooth, elliptical morphology, while the other has an asymmetrical shape with more defined features. There appears to be an off-centered, point-like nucleus associated with the smoother component. The apparent asymmetry may indicate tidal disruption. There is a gradient in color from the central region of the galaxy to the edges of the halo. There is also a strong green color to the extended halo of the galaxy.
