The observed galaxy presents as an edge-on spiral galaxy with a redshift of approximately 0.154, suggesting a considerable distance. The galaxy displays a prominent disk structure, viewed almost perfectly edge-on. A central bulge is visible, appearing somewhat rounded in morphology, and likely hosts a supermassive black hole. The galaxy's disk exhibits a relatively smooth appearance, with minimal evidence of strong spiral arm structure or significant dust lane obscuration. The integrated color suggests a galaxy that is actively forming stars, though not at an exceedingly high rate. There is no evidence of major mergers or strong tidal disturbances, although some minor disturbances cannot be ruled out given the resolution. Based on its absolute magnitude, the galaxy appears to be relatively luminous. Overall, this galaxy appears to be a fairly typical edge-on spiral galaxy at intermediate redshift, exhibiting ongoing star formation and a relatively undisturbed morphology.
