The galaxy exhibits a complex morphology, appearing to be in a late stage interaction or merger. The overall structure is highly disturbed, lacking a clearly defined spiral or elliptical form. A prominent, elongated feature with intense star formation is visible. This region displays a gradient in color, suggesting differing stellar populations or dust content along its length. One of the merging galaxies appears to have a fairly compact center. Star formation is suppressed, but has occurred in the past. There appears to be a tidal tail or stream of material extending away from the main body, indicating strong gravitational interactions. Overall, the galaxy system shows significant evidence of recent or ongoing dynamical processes.
