The galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms are tightly wound and traced by regions of active star formation. These star-forming regions appear as faint blue knots along the arm segments. The arms originate from a central bulge, which appears to be moderate in size. The bulge region exhibits a more yellow-white coloration, potentially indicating an older stellar population.

The galaxy has a slight inclination with respect to our line of sight, allowing a partial view of its disk. No significant signs of ongoing major merger activity are visible in the galaxy's morphology, although there may be minor disturbances within the disk. A bar structure appears to exist across the galactic nucleus, with a noticeable presence. The light distribution indicates a more elongated shape. Overall, the galaxy exhibits a classic spiral morphology with evidence of a relatively high inclination angle.
