The galaxy appears to be undergoing a significant merger event. Two distinct luminous components are visible, seemingly in the late stages of interaction. Each component exhibits an ellipsoidal morphology, though distorted from a perfectly smooth shape. There is a noticeable tidal bridge of luminous material connecting the two main bodies. The color indices suggest an older stellar population, with redder colors predominating throughout the system. The overall structure is highly disturbed, indicating ongoing gravitational interactions. The system appears to be relatively massive, with a faint extended halo surrounding the main bodies. The rate of star formation appears to be reduced, indicating a more evolved system.
