The galaxy presents a disk-like structure, exhibiting a distinct spiral morphology. A moderate bulge is visible at the center, appearing yellowish in color, which suggests an older stellar population. The spiral arms extend outwards from the central bulge region. The arms display a somewhat tightly wound structure. These arms appear clumpy, indicating regions of active star formation. The overall color of the disk shows a blueish tint which would suggest a younger stellar population than the central bulge. The galaxy does not show any obvious signs of major interaction or disturbance based on the morphology of its arms. The orientation of the galaxy appears to be more face-on, allowing for detailed observation of the spiral structure.
