  Noncommutative geometry is an established potential candidate for including
quantum phenomena in gravitation. We outline the formalism of Hopf algebras and
its connection to the algebra of infinitesimal diffeomorphisms. Using a
Drinfeld twist we deform spacetime symmetries, algebra of vector fields and
differential forms leading to a formulation of noncommutative Einstein
equations. We study a concrete example of charged BTZ spacetime and
deformations steaming from the so called angular twist. The entropy of the
noncommutative charged BTZ black hole is obtained using the brick-wall method.
We used a charged scalar field as a probe and obtained its spectrum and density
of states via WKB approximation. We provide the method to calculate corrections
to the Bekenstein-Hawking entropy in higher orders in WKB, but we present the
final result in the lowest WKB order. The result is that even in the lowest
order in WKB, the entropy, in general, contains higher powers in $\hbar$, and
it has logarithmic corrections, and polynomials of logarithms of the black hole
area.
