The galaxy appears to be a spiral galaxy, observed at an oblique angle. The presence of spiral arms is subtly suggested by variations in color and brightness across the galactic disk, particularly in the blue light spectrum. The galaxy exhibits a noticeable central bulge, with a concentration of light. This region is more yellow in hue compared to the bluer arms, indicating an older stellar population. The disk appears relatively thin. There may be a faint bar feature present across the galaxy. Overall, the galaxy displays signs of active star formation, evidenced by the presence of blue regions along the spiral arms.
