The observed galaxy presents a morphology characteristic of a spiral galaxy with a prominent central bulge. Spiral arms are clearly visible, displaying a grand design structure with well-defined winding. The arms exhibit a loose to medium pitch angle, suggesting ongoing star formation activity within the spiral arms as evidenced by their bluer coloration. The bulge appears moderately sized and exhibits a yellowish-white hue, indicative of an older stellar population. The disk component displays a relatively high inclination angle, but is not quite edge-on. There is evidence of mild gravitational disturbance in the galactic structure, but the overall spiral structure remains largely intact. Overall, the galaxy presents a classic spiral morphology.
