The galaxy presents as a thin, elongated disk, viewed nearly edge-on. There is a prominent central bulge, brighter and more concentrated than the disk. The bulge appears to be primarily of a rounded morphology. The disk itself shows a subtle color gradient, with bluish-white hues apparent in the outer regions, suggesting recent star formation. Darker dust lanes are hinted at within the disk, obscuring some of the light. Faint, diffuse emission extends away from the main body of the galaxy, potentially indicating a halo structure or tidal features from a past interaction. The system appears to be relatively undisturbed, displaying no obvious signs of a recent major merger, however, it is unclear if there are minor tidal disturbances.
