The galaxy presents a distinct spiral morphology. The spiral arms are apparent but are tightly wound, exhibiting a flocculent structure with substantial patchiness. There is evidence of multiple arm structures, with at least three arms discernible. The central bulge appears relatively small and unresolved. The disk of the galaxy is viewed close to face-on. The galaxy has clumpy star formation regions with a blue hue, tracing the spiral arms. A slight disturbance in the morphology suggests a potential minor gravitational interaction or merger event. There is also evidence of a bar structure spanning through the center of the galaxy, but it does not appear to be prominent.
