This galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction. The light distribution is not smooth and shows evidence of tidal features. There are two distinct bright nuclei, with a stream of fainter material connecting them. The main body of the galaxy is elliptical in shape. Color gradients are present, with a more yellow-red central region, indicating a possibly older stellar population. The periphery shows signs of bluer light, which could indicate ongoing or recent star formation. 
