The galaxy displays a disk morphology with prominent spiral arms. The spiral arms are loosely wound and extend noticeably from the central region. There are two clearly defined spiral arms. A prominent bar structure appears to bisect the central bulge, which seems to be of moderate size. There is evidence of a significant interaction or merger event. One of the arms is slightly distorted and there may be tidal tails. The color suggests active star formation is present within the spiral arms, with regions of bluer light scattered throughout the disk.
