The galaxy appears to be undergoing a significant merging event. Two distinct nuclei are visible, both exhibiting a bright, yellowish-white color, suggesting an older stellar population is dominant. The morphology indicates a relatively smooth overall structure, but with clear signs of disturbance and interaction. The system is moderately luminous, with a compact size indicating it is relatively close in astronomical terms. There is some evidence of faint tidal features, but no well-defined spiral arms or a prominent disk. The color suggests that ongoing star formation is likely suppressed, indicating that the system is possibly evolving into an elliptical galaxy. 
