  We study the asymptotic quasi-normal modes for the scalar perturbation of the
non-commutative geometry inspired Schwarzschild black hole in (3+1) dimensions.
We have considered $M\geq M_0$, which effectively correspond to a single
horizon Schwarzschild black hole with correction due to non-commutativity. We
have shown that for this situation the real part of the asymptotic quasi-normal
frequency is proportional to $\ln (3)$. The effect of non-commutativity of
spacetime on quasi-normal frequency arises through the constant of
proportionality, which is Hawking temperature $T_H(\theta)$. We also consider
the two horizon case and show that in this case also the real part of the
asymptotic quasi-normal frequency is proportional to $\ln(3)$.
