The galaxy presents a morphology consistent with a spiral galaxy. The disk appears nearly face-on. Spiral arms are visible, exhibiting a somewhat flocculent structure, and spanning a significant portion of the galaxy's radius. A central bulge component is discernible, though it does not appear to dominate the overall structure. The disk shows signs of some asymmetric structures, potentially indicative of minor interactions or internal instabilities. There appears to be a bar-like feature extending through the center of the bulge. There is little apparent evidence of active merging or major tidal disturbances affecting the system.
