  We narrate dark matter, neutrino magnetic moment and mass in a Type-III
radiative scenario. The Standard Model is enriched with three vector-like
fermion triplets and two inert doublets to provide a suitable platform for the
above phenomenological aspects. The inert scalars contribute to total relic
density of dark matter in the Universe. Neutrino aspects are realized at
one-loop with magnetic moment obtained through charged scalars, while neutrino
mass gets contribution from charged and neutral scalars. Taking inert scalars
up to $2$ TeV and triplet fermion in few hundred TeV range, we obtain a common
parameter space, compatible with experimental limits associated with both
neutrino and dark matter sectors. Using a specific region for transition
magnetic moment (${\cal O} (10^{-11}\mu_B$)), we explain the excess recoil
events, reported by the XENON1T collaboration. Finally, we demonstrate that the
model is able to provide neutrino magnetic moments in a wide range from
$10^{-12}\mu_B$ to $10^{-10}\mu_B$, meeting the bounds of various experiments
such as Super-K, TEXONO, Borexino and XENONnT.
