This galaxy exhibits an elongated, irregular morphology. The primary structure appears to be a distorted or disrupted disk, with a noticeable extension in one direction. There is evidence of possible tidal features, suggesting an interaction or merger event with another galaxy, or potentially a recent internal disturbance. The color gradient suggests an older stellar population throughout the main body, with regions of more active star formation concentrated in distinct, somewhat knotty regions. Overall, the galaxy presents a disturbed and potentially evolving system.
