The galaxy presents as an edge-on spiral, displaying a prominent, relatively large, and elongated disk structure. The dust lane is significant, bisecting the galaxy along its major axis and obscuring a portion of the galactic bulge. The bulge itself appears smooth and rounded. There is no obvious sign of a bar structure or spiral arm detail due to the edge-on orientation. The overall color of the galaxy is yellowish, suggesting a dominant population of older stars. There are no obvious signs of recent major merger activity or tidal disturbances. Some minor disturbances may exist but cannot be confidently confirmed. The galaxy's structure suggests that this galaxy is composed of roughly 10^10 solar masses. Star formation may be present, but likely at a low rate.
