This galaxy appears to be undergoing a significant merger event. Two distinct nuclei are visible, one slightly larger and more reddish in color than the other. The overall morphology is disturbed and asymmetrical, lacking a clear spiral or elliptical structure. The light distribution suggests a relatively smooth profile dominated by an older stellar population. Star formation activity is likely occurring, but at a low rate given the high level of red light and small amount of blue light. The estimated size of the galaxy is relatively compact. The nuclei of the galaxy are also very round.
