The galaxy presents a spiral morphology with prominent, well-defined spiral arms. The disk component dominates the structure. The central bulge appears relatively small and faint, suggesting a lower concentration of older stars compared to the disk. The galaxy is not seen edge-on but at a relatively high inclination angle, allowing the spiral structure to be readily observed. A weak bar structure may be present in the center, with a subtle elongation noted. There are signs of minor disturbances but the overall structure is still very recognizable, so a major merging event is unlikely.
