The galaxy presents a distinct spiral structure, though the spiral arms appear tightly wound. The arms are traced by regions of blue light, suggesting active star formation within these areas. A prominent central bulge is visible, exhibiting a yellowish-white hue that likely indicates an older stellar population. The galaxy is oriented nearly face-on. Overall, there is no obvious sign of major mergers, though minor disturbances cannot be ruled out. A population of dust is likely present throughout the galaxy, due to the redness of the stars.