The observed galaxy presents a clear edge-on disk morphology. Dust lane obscuration is readily apparent, bisecting the central region along the major axis. The bulge is not prominent and difficult to resolve, appearing small and unobtrusive, seemingly lacking a distinct or boxy shape. The disk exhibits a smooth texture, indicating a lack of substantial, large-scale star-forming regions visible in the imaging. There is no evidence of ongoing major mergers or significant tidal disturbances to its form. The overall color profile implies intermediate star formation activity. The light distribution appears relatively uniform across the visible disk.
