The galaxy exhibits a somewhat disturbed morphology, suggestive of a possible interaction or merger event. Its overall color is yellowish-orange, indicative of an older stellar population with diminished recent star formation. Some regions display a smoother appearance, while others show evidence of more complex features, possibly disrupted spiral arms or tidal tails. There is a slightly elongated central region that is indicative of a disk. Overall the galaxy seems to be undergoing some form of merger.
