The galaxy presents as a highly inclined, disk-shaped system. Dust lanes are subtly visible, particularly along the major axis, contributing to an observed reddening of the central region. The galaxy exhibits a bright central bulge, with luminosity decreasing significantly toward the outer edges of the disk. Some blue coloration is present, especially in the outer regions, suggestive of some ongoing star formation. The disk shows some faint, flocculent spiral arm structure, though the high inclination makes precise morphological classification challenging. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of major mergers or interactions.
