  We investigate neutrino magnetic moment, triplet scalar dark matter in a
Type-II radiative seesaw scenario. With three vector-like fermion doublets and
two scalar triplets, we provide a loop level setup for the electromagnetic
vertex of neutrinos. All the scalar multiplet components constitute the total
dark matter abundance of the Universe and also their scattering cross section
with detector lie below the experimental upper limit. Using the consistent
parameter space in dark matter domain, we obtain light neutrino mass in sub-eV
scale and also magnetic moment in the desired range. We further derive the
constraints on neutrino transition magnetic moments, consistent with XENONnT
limit.
