The galaxy presents a morphology indicative of a system undergoing, or having recently undergone, a major merger event. There appear to be two distinct nuclei present within a common halo of diffuse light. The nuclei display a yellowish-orange hue. One nucleus appears slightly brighter and more compact than the other. The overall shape of the galaxy is somewhat elongated and irregular. There is evidence of tidal disturbances or extended structures beyond the main body of the galaxy, indicative of gravitational interactions. While much of the light from the central area of the galaxy is reddish yellow, implying a slightly older stellar population, some bluer regions can be seen surrounding the nucleus on the left, suggesting possible regions of recent star formation.
