The galaxy exhibits a clear spiral structure. The spiral arms are well-defined and appear somewhat patchy, indicating areas of differing stellar density or dust obscuration. The arms seem to wind moderately tightly around the central bulge. The bulge is a significant feature, appearing relatively bright and yellow, suggesting an older stellar population. There is no obvious presence of a central bar structure within the galaxy. The overall shape indicates a grand-design spiral, not obviously disturbed, though subtle irregularities within the arm structure may hint at minor interactions. Evidence of active star formation is visible in the arms.