The galaxy presents as a spiral with a notably bright central bulge, indicating a concentration of older stellar populations. Faint spiral arms extend from the central region, though they appear somewhat diffuse and lack sharp definition. There is evidence of ongoing, but not particularly vigorous, star formation as indicated by the slightly bluer tinge within the arms. The galaxy exhibits a disk-like structure, with an approximate diameter of roughly 9 kpc. Overall, the galaxy appears relatively undisturbed, without obvious signs of major mergers, although some minor distortions in the outer disk cannot be ruled out. The galaxy has an estimated stellar mass of approximately 10^10 solar masses.
