  We propose to accommodate economically the type-II neutrino seesaw mechanism
in (G)NMSSM from GMSB and AMSB, respectively. The heavy triplets within
neutrino seesaw mechanism are identified to be the messengers. Therefore, the
$\mu$-problem, the neutrino mass generation, LFV as well the soft SUSY breaking
parameters can be economically combined in a non-trivial way. General features
of such extensions are discussed. The type-II neutrino seesaw-specific
interactions can give additional Yukawa deflection contributions to the soft
SUSY breaking parameters of NMSSM, which are indispensable to realize
successful EWSB and accommodate the 125 GeV Higgs. Relevant numerical results,
including the constraints of dark matter and possible LFV processes
$l_i\rightarrow l_j \gamma$ etc, are also given. We find that our economical
type-II neutrino seesaw mechanism extension of NMSSM from AMSB or GMSB can lead
to realistic low energy NMSSM spectrum, both admitting the 125 GeV Higgs as the
lightest CP-even scalar. The possibility of the 125 GeV Higgs being the
next-to-lightest CP-even scalar in GMSB-type scenario is ruled out by the
constraints from EWSB, collider and precision measurements. The possibility of
the 125 GeV Higgs being the next-to-lightest CP-even scalar in AMSB-type
scenario is ruled out by dark matter direct detection experiments. Possible
constraints from LFV processes $l_i\rightarrow l_j \gamma$ can give an upper
bound for the messenger scale.
