The galaxy exhibits a morphology suggesting an ongoing or recent merger event. The primary structure displays a generally smooth appearance but appears to have two distinct centers of luminosity. The primary body of the galaxy shows a color gradient, trending toward a yellow/orange hue in the denser central regions. The overall shape is somewhat round with no strong indication of spiral arms. The color suggests a population of older stars, possibly indicating a relatively quiescent star formation rate. Some structural distortion is visible, lending further evidence to a merger event. 
