  In this paper, we analyze the symmetry properties of the complete family of
type D spacetimes generalized form the Pleba\'{n}ski-Demia\'{n}ski solution in
four dimensions holographically in terms of a warped CFT. The generalized
Pleba\'{n}ski-Demia\'{n}ski solutions are black hole-like spacetimes
characterized by seven physical parameters. Most of the black holes in four
dimensions are included within this family. Generically consider a solution
with horizon in this family, we figure out the possible warped conformal
symmetry attached to the horizon. The horizon can be either extremal or
non-extremal. In the extremal case, the near horizon region can be mapped to an
infinite spacetime with geometry given by a warped and twist product of AdS$_2$
and S$^2$. The new boundary conditions for AdS$_2$ as well as their higher
dimensional uplifts are applied here to manifest the asymptotic symmetry as the
warped conformal symmetry. In the non-extremal case, the global warped
conformal symmetry is singled out by analyzing the scalar wave equation with
constant frequency. The local warped conformal symmetries are represented by
the charge algebra associated to the vector fields which preserve the scalar
wave equation as well as its frequency. In defining the variation of the
covariant charges, a proper counterterm is introduced for consistency
conditions which is supposed to be suitable for all the solutions within the
family. As a consistency check, the horizon entropy is reproduced by the
entropy formula of the warped CFT by using its modular covariance and the
central terms derived in the bulk spacetimes.
