The galaxy presents as a system undergoing a significant merger. One of the merging galaxies exhibits a roughly elliptical morphology with a concentrated central bulge and a smooth appearance with a predominantly orange hue. The other merging component appears as a more diffuse, less structured object exhibiting a similar reddish color. There appears to be tidal distortion and extended faint emission emanating from the larger galaxy, suggesting gravitational interaction between the two components. The tidal features are quite faint, indicating a possible later stage of merging. The overall system displays a relatively smooth profile suggesting an evolved system. Evidence suggests low star formation rates and low specific star formation rates.
