  Using a model of an accretion disk around a Schwarzschild black hole, the
analytic estimates for image polarization were derived by Narayan $et~al.$.
[Astrophys. J, 102, 912 (2021)]. Recently, the EHT team also obtained
polarization images of the Sgr A$^{*}$ and measured both linear and circular
polarization [Astrophys. J. Lett, 964, L25 (2024)]. We find that quantum
correction effects can also influence polarization information. Considering the
quantum corrected Schwarzschild black hole (Kazakov-Solodukhin black hole), we
derive the polarization intensity of the target black hole and investigate
polarization images under different parameters. It is found that a larger
quantum deformation leads to an expansion of the polarization region, while the
polarization intensity value decrease. Under different observation angles,
magnetic fields, fluid direction angles, and fluid velocity conditions, we also
derive polarization images of corrected black holes. These key indicators not
only affect the intensity of polarization but also the direction of
polarization. We establish the relationship between polarization intensity and
quantum correction deformation parameters, revealing a gradual decline in
polarization intensity with reduced radius and an anti-polarization behavior
induced by the progressive increase in deformation parameters at a constant
radius. Our analysis may provide observational evidence for quantum effect of
general relativity.
