This galaxy exhibits a clear spiral structure. The spiral arms are prominent but somewhat tightly wound and well-defined. Two dominant arms are observed. There is evidence of a central bulge, appearing moderately sized relative to the disk. A bar structure is present, extending from the center. The galaxy shows minimal signs of significant tidal disturbances or ongoing major mergers, although there may be minor irregularities in the spiral arm structure suggesting past interaction or minor disturbances. Dust lanes are visible within the spiral arms. Overall, the galaxy appears as a relatively undisturbed spiral galaxy.
