This galaxy appears to be undergoing a significant merger event. Two distinct, bright nuclei are visible, indicating the presence of two interacting galaxies. The overall morphology of the system is highly disturbed, with a diffuse halo of stellar material surrounding the nuclei. There is evidence of tidal features, suggesting gravitational interactions are actively reshaping the galactic structure. The color gradient suggests relatively mature stellar populations, possibly indicating a lower rate of star formation within the main bodies. The central regions display warmer colors compared to the outer halo. Overall, this galaxy is dynamically active due to the ongoing merger.
