  In this paper, we aim to explore the impact of the Planck scale corrections
and the Holographic quintessence on the shadow behavior of non-rotating black
holes. To do this, we consider the quantum-corrected Schwarzschild black hole
surrounded by the quintessence field inspired by the Kazakov-Solodukhin and the
Kiselev ideas, and we call this combination the Kazakov-Solodukhin-Kiselev
(KSK) black hole. We conclude that the quintessence field as the candidate of
dark energy in the black hole can be interpreted as Holographic quintessence.
To find the geodesic equations of the black hole, we employ the Hamilton-Jacobi
approach and also, the Carter procedure. We discover that the size of the
shadow of this black hole, which depends on its central mass, is also
determined by the Planck scale effects and Holographic quintessence.
