This galaxy appears to be undergoing a significant merger event. Two distinct nuclei are visible, suggesting the recent collision of two galaxies. The overall shape is irregular and disturbed, lacking a defined disk or spiral structure. The color distribution is complex, with regions of reddish hues potentially indicating older stellar populations, and greenish tinges possibly associated with regions of ongoing star formation. The system is compact, with no obvious tidal tails or extended features, suggesting that the merger is relatively early in its progression. Overall, this appears to be a luminous interacting system with strong evidence of gravitational disturbance.
