  We point out that the Cabibbo-Kobayashi-Maskawa (CKM) quark mixing matrix
$V_{\rm CKM}$ and the Maki-Nakagawa-Sakata (MNS) lepton mixing matrix $V_{\rm
MNS}$ can naturally be correlated in a class of seesaw models with grand
unification, but the texture of their correlation matrix ${\cal F}_\nu$ is
rather nontrivial. The bimaximal mixing pattern of ${\cal F}_\nu$ is disfavored
by current data, and other special forms of ${\cal F}_\nu$ may suffer from
fine-tuning of the free phase parameters in fitting the so-called quark-lepton
complementarity relation. A straightforward calculation of ${\cal F}_\nu$ in
terms of $V_{\rm CKM}$ and $V_{\rm MNS}$ reveals a striking feature of ${\cal
F}_\nu$: its (1,3) element cannot be zero or too small, no matter whether the
(1,3) elements of $V_{\rm CKM}$ and $V_{\rm MNS}$ are vanishing or not. We also
add some brief comments on possible radiative corrections to $V_{\rm CKM}$ and
$V_{\rm MNS}$.
