This galaxy presents as a distorted spiral form, exhibiting clear signs of disruption. There appears to be a central bulge which seems to be moderately pronounced, which could indicate a small supermassive black hole in the center. Spiral arms extend from the central region, but they display asymmetry and clumpy structures, hinting at ongoing or past interactions. Some areas of the arms seem to be more luminous than others. The arms are not smoothly distributed. Based on the morphology, the galaxy is likely undergoing a minor merger or experiencing some sort of gravitational disturbance. Furthermore, a weak bar structure may be present, slightly elongated through the center of the galaxy. A higher resolution image would give greater insight.
