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The quasar images, produced by a foreground cluster of galaxies, have a maximum separation angle of theta similar to 22 \u0027\u0027.5. The large angular separation suggests that the sight lines to the quasar central source can go through different regions of outflowing winds from the accretion disk of the quasar, providing a unique opportunity to study the structure of outflows from the accretion disk, a key ingredient for the evolution of quasars as well as for galaxy formation and evolution. Based on medium- and high-resolution spectroscopy of the two brightest images conducted at the Subaru telescope, we find that each image has different intrinsic levels of absorptions, which can be attributed either to variability of absorption features over the time delay between the lensed images, Delta t similar to 744 days, or to the fine structure of quasar outflows probed by the multiple sight lines toward the quasar. 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The quasar images, produced by a foreground cluster of galaxies, have a maximum separation angle of theta similar to 22 \u0027\u0027.5. The large angular separation suggests that the sight lines to the quasar central source can go through different regions of outflowing winds from the accretion disk of the quasar, providing a unique opportunity to study the structure of outflows from the accretion disk, a key ingredient for the evolution of quasars as well as for galaxy formation and evolution. Based on medium- and high-resolution spectroscopy of the two brightest images conducted at the Subaru telescope, we find that each image has different intrinsic levels of absorptions, which can be attributed either to variability of absorption features over the time delay between the lensed images, Delta t similar to 744 days, or to the fine structure of quasar outflows probed by the multiple sight lines toward the quasar. 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