This galaxy appears to be undergoing a significant interaction or merger. The morphology is disturbed, exhibiting an irregular shape with a suggestion of two distinct, luminous cores. These cores are bright and yellowish in color, potentially indicating older stellar populations, though obscured star formation cannot be ruled out. There is some faint, extended emission surrounding the central region, but the overall structure lacks well-defined spiral arms or a smooth elliptical profile. The overall color suggests a more evolved system, but the disturbed morphology hints at recent or ongoing dynamical activity.
