The galaxy presents as a face-on spiral, with a noticeable central bulge that is more subdued than dominant. Distinct spiral arms emanate from the bulge, displaying a range of winding tightness. The galaxy exhibits a bar-like structure crossing its central region, more easily identified as weak but evident. The arm count appears to favor a two-arm morphology, potentially accompanied by a structure that is either merging or experiencing some form of gravitational disturbance.
