This galaxy exhibits a clear spiral structure, with prominent arms that appear somewhat flocculent. The central bulge is bright and concentrated. Dust lanes are visible in the spiral arms, appearing as dark regions silhouetted against the brighter starlight. The spiral arms display a moderate winding, neither tightly wound nor fully open, and a grand-design, two-arm structure appears to dominate the disk. No strong bar structure is apparent. There are no obvious signs of major merger events or significant tidal disturbances. The galaxy seems relatively isolated, displaying a classic spiral morphology with a moderate-sized bulge and active star formation in the spiral arms. The galaxy is inclined slightly from our viewpoint, appearing almost face-on.
