The galaxy appears to be undergoing a significant merger event. Two distinct luminous regions are visible, suggesting the presence of two galactic nuclei in close proximity. A considerable amount of tidal distortion is evident, indicated by the overall amorphous shape of the galaxy. The primary light emitted appears yellowish-orange, possibly indicating an older stellar population, although some regions show a hint of bluer light indicating the presence of some young stars. The morphology leans toward a smooth profile with disturbances and tidal features. The two nuclei are surrounded by diffuse light, which appears to be interacting.
