  {In (Sci. Rep. \textbf{12}, 8516 (2022)), Campos et al studied} the
quasinormal modes and shadows of noncommutative Schwarzschild black holes.
Since we know that the quintessence matter surrounding black holes has {
significant effects} on the black hole quantities, {in this study, we aimed to
show this influence by revisiting the same problem in the presence of
quintessence matter field. To this end, we first examined the thermodynamics of
noncommutative Schwarzschild black holes embedded in quintessence matter using
Hawking temperature, entropy, and specific heat functions. After that,} we
discussed phase transition and stability { features. We then investigated} the
shadow images in the presence of plasma. After visualizing these results
qualitatively, we calculated the quasinormal modes in WKB and Mashhoon
approximations and we demonstrated the impacts of quintessence matter and
noncommutative spacetime on the whole quantities.
