  In this manuscript, we investigate the extended uncertainty principle (EUP)
effects on the Van der Waals (VdW) black holes whose thermal quantities mimic
the VdW liquid. We find that the considered formalism imposes an upper bound on
the event horizon radius. Thus, the mass, Hawking temperature, and heat
capacity become physically meaningful within a certain range of event horizon
radii. At a large event horizon radius the black hole has a remnant. We observe
that for a given set of parameters, the VdW black hole can be completely
unstable for all horizon radii, while for another set of parameters, it can be
unstable or stable depending on the horizon radius.
