The galaxy presents a morphology suggestive of an ongoing or recent merger event. Two distinct, bright nuclei are visible, each exhibiting a yellowish-orange hue, likely indicating an older stellar population. A faint, diffuse envelope surrounds both nuclei, with potential tidal features or disturbed morphology suggesting gravitational interaction. The galaxy appears to be relatively compact, and is roughly in between round and cigar-shaped. There is not significant evidence of star formation given the lack of bluish colors.
