This galaxy presents a morphology consistent with a spiral galaxy, viewed at a slight angle relative to face-on. The central region exhibits a notable bulge component, appearing relatively smooth and concentrated. Surrounding the bulge, distinct spiral arms extend outward, displaying a flocculent structure with a moderate pitch angle. The arms appear somewhat tightly wound. Patches of bluer light indicate areas of active star formation within the spiral arms. There is no obvious signs of a strong bar structure, or major disturbances indicating ongoing or recent merger activity. Overall, the galaxy demonstrates a well-defined disk with a prominent spiral arm pattern.