  In this manuscript, we examine the Schwarzschild black hole surrounded by
perfect fluid dark matter in the presence of the quintessence matter field in
the context of thermodynamics, shadows, and quasinormal modes. We find that the
quintessence matter field sets an upper bound value on the horizon where dark
matter settles a lower limit on the event horizon but also expands the upper
bound value of the horizon. We discuss how this impact alters the black hole's
thermodynamics, shadows, and quasinormal modes.
