The galaxy appears to be in a late-stage merger event, exhibiting a highly disturbed morphology. Two distinct luminous cores are readily apparent, suggesting the presence of two progenitor galaxies interacting gravitationally. Tidal features are prominent, displaying extended faint light extending from the main bodies. There is possible evidence of dust lanes in the galactic center. The system displays a generally red color profile. Based on the smooth and round nature of the merger, it is likely to evolve into an elliptical galaxy.
