  In this work we investigate a Schwarzschild-type black hole that is corrected
by the Generalized Uncertainty Principle (GUP) and possesses topological
defects within the framework of Bumblebee gravity. Our focus is on the
thermodynamic characteristics of the black hole, such as temperature, entropy
and heat capacity, which vary as functions of the horizon radius, and also on
shadow as an optical feature. Our investigation reveals significant changes in
the thermodynamic behavior of the black hole due to violations of Lorentz
symmetry, GUP corrections, and the presence of monopoles. However, the shadow
of the black hole is unaffected by violations of Lorentz symmetry. In addition,
we provide a limit on the parameters of Lorentz symmetry violation, GUP and
topological defects based on a classical test involving the precession of
planetary orbits and the advancement of perihelion in the solar system.
