The galaxy appears to be in a late stage of merging. The primary body of the galaxy exhibits a smooth, somewhat irregular morphology, suggesting an elliptical-like shape. Evident tidal features distort the overall structure, indicating significant gravitational interaction with the other body. Blue-ish and white hues are prevalent throughout the center of the disk, this may indicate ongoing star formation within the disk. The second body of the galaxy appears to be much smaller and closer to a spherical-like shape. Overall, the system shows clear signs of disturbance and active merging.
