The observed galaxy presents a spiral morphology, exhibiting prominent, well-defined spiral arms. These arms appear loosely wound and extend outwards from a central region. The central bulge component is readily visible, demonstrating a moderate size relative to the overall galactic disk, displaying a gradual transition into the spiral arms. The presence of several star-forming regions is suggested by the mottled texture observed within the spiral arms, with varying degrees of brightness and color, indicating differing stellar populations and dust content. There is no apparent strong central bar, suggesting a non-barred spiral classification. The disk is observed nearly face-on. Some evidence of gravitational disturbance is observable in the asymmetry and clumpy structure of the outer arms, possibly indicating a recent interaction. The galaxy appears to be undergoing a period of active star formation.
