The galaxy appears to be undergoing a major merger event. Two distinct nuclei are visible, separated by what appears to be tidal debris. The nuclei exhibit a reddish-orange hue, suggesting an older stellar population.  The overall color of the galaxy is reddish, further indicating a potentially low star formation rate.  There are faint hints of blueish diffuse light extending away from the primary merging components, possibly indicative of tidal tails. The galaxy shows clear signs of morphological disturbance. The light distribution is not smooth and there are irregular features.
