The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. Two distinct luminosity peaks are observed, one of which is more diffuse and yellowish and the other which is tighter and blueish in color. There is likely significant tidal disruption present. The galaxy is relatively compact. The overall light profile appears moderately smooth, but with clear irregularities indicative of gravitational interactions. The red color observed may be from older stars or dust reddening from the on going merger, while the bluer components of the galaxy suggest ongoing star formation.
