  Residual symmetry $G_\nu$ of neutrino mass matrix with a massless neutrino
and embedding of $G_\nu$ and the residual symmetry $G_l$ of the charged lepton
mass matrix into finite discrete groups $G$ is discussed. Massless neutrino
results if $G_\nu$ and hence $G$ are subgroups of $U(3)$ rather than of
$SU(3)$. Structure of the resulting leptonic mixing matrix $U_{PMNS}$ is
discussed in three specific examples based on groups (a) $\Sigma(3N^3)$, (b)
$\Sigma(2N^2)$ and (c) $S_4(2) \equiv A_4\rtimes Z_4$. $\Sigma(3N^3)$ groups
are able to reproduce either the second or the third column of $U_{PMNS}$
correctly. $\Sigma(2N^2)$ groups lead to prediction $\theta_{13}=0$,
$\theta_{23}=\frac{\pi}{4}$ for the reactor and atmospheric mixing angles
respectively if neutrino mass hierarchy is inverted. Solar angle remains
undetermined in this case. This also gets determined when $G=S_4(2)$ which can
give bi-maximal mixing for inverted hierarchy. Examples (b) and (c) provide a
good zeroth order approximation to realistic leptonic mixing with a massless
neutrino. We also present an example of the specific model based on $S_4(2)$
symmetry in which a massless neutrino and viable leptonic mixing angles are
obtained.
