  We discuss some thermodynamic properties as well as the stability of a
quantum Schwarzschild black hole, comparing the results with those obtained
within a bumblebee gravity model. In particular, the Hawking temperature,
$T_H$, the entropy, $S$, the heat capacity, $C$, and the Gibbs free energy,
$G$, are computed for both cases. In addition to that, we compute the
Brown-York quasilocal energy and compare the solution with the Schwarzschild
case. We find that in both cases (quantum Schwarzschild and bumblebee gravity
model) the temperature, the entropy, and the heat capacity show the same
functional form, under the replacement $\lambda^2 \rightarrow \ell$ and vice
versa. Specifically, the temperature is found to be lower compared to the
classical (Schwarzschild) solution, whereas the entropy is computed to be
larger. Moreover, the heat capacity becomes more negative. Notably, a distinct
contrast emerges in obtaining the Gibbs free energy between these two cases,
and this distinction appears to stem from the ADM mass.
