  Fermi J1544-0649 is a transient GeV source first detected during its GeV
flares in 2017. Multi-wavelength observations during the flaring time
demonstrate variability and spectral energy distribution(SED) that are typical
of a blazar. Other than the flare time, Fermi J1544-0649 is quiet in the GeV
band and looks rather like a quiet galaxy (2MASX J15441967-0649156) for a
decade. Together with the broad absorption lines feature we further explore the
"misaligned blazar scenario". We analyzed the Very Long Baseline Array (VLBA)
and East Asian VLBI Network (EAVN) data from 2018 to 2020 and discovered the
four jet components from Fermi J1544-0649. We found a viewing angle around
3.7{\deg} to 7.4{\deg}. The lower limit of the viewing angle indicates a blazar
with an extremely low duty cycle of the gamma-ray emission, the upper limit of
it supports the "misaligned blazar scenario". Follow-up multi-wavelength
observations after 2018 show Fermi J1544-0649 remains quiet in GeV, X-ray, and
optical bands. Multi-messenger search of neutrinos is also performed, and an
excess of 3.1 {\sigma} significance is found for this source.
