This galaxy exhibits a distinct spiral structure with well-defined arms. The arms appear somewhat flocculent, showing a patchy distribution of star formation. The galaxy presents a moderate inclination to our line of sight. A central bulge is present, though it does not dominate the overall structure. The spiral arms exhibit a moderate winding, with a noticeable population of young, blue stars within them, indicating ongoing star formation. Dust lanes are visible, particularly on the near side of the galaxy, obscuring some of the starlight. A bar structure is evident within the central region, potentially influencing the spiral arm morphology. The galaxy displays an overall asymmetric distribution of light, with a slightly elongated shape. There may be some minor disturbances visible, possibly indicating past or ongoing interactions with other galaxies.
