The galaxy exhibits a prominent disk structure with a moderate inclination relative to our line of sight. Within the disk, spiral arm features appear present but somewhat indistinct, exhibiting a flocculent or patchy morphology. A central bulge is clearly visible, with a moderate size compared to the overall disk. The bulge displays a yellowish-white color, suggesting an older stellar population.

Evidence of a bar structure is present. The overall shape of the galaxy is symmetrical, with no obvious signs of a major ongoing merger event, however, there may be minor disturbances. The disk shows a gradient in color, bluer towards the outer regions, indicating younger stars and active star formation. The disk is relatively smooth, and lacks intense star-forming regions.
