The galaxy presents as a grand design spiral with a notable central bulge. Its spiral arms are tightly wound, displaying a high degree of symmetry. There is a pronounced concentration of older stars near the galactic nucleus, indicated by a yellowish hue in the central bulge. The spiral arms exhibit a bluer color, suggesting ongoing star formation. Faint dust lanes can be seen along the inner edges of some spiral arms. The disk of the galaxy is relatively thin. The galaxy is not undergoing any major mergers or interactions, though it displays minor disturbances. Based on these features, the galaxy is likely a mature spiral galaxy undergoing steady star formation.
