The galaxy presents a defined disk-like structure, with prominent spiral arms. These arms display a loosely wound morphology. Evidence suggests that the galaxy is experiencing significant star formation, as traced by bluer colors within the spiral arms. A central bulge region is visible, exhibiting a yellowish hue indicative of an older stellar population. There is a suggestion of a bar-like structure spanning across the central region of the galaxy. Overall, the galaxy exhibits a grand design spiral morphology. A slight disturbance in the outer disk suggests a past or ongoing minor interaction or merger event. 
