  We report the results of optical spectroscopy of the candidate evolved
massive star MN44 revealed via detection of a circular shell with the Spitzer
Space Telescope. First spectra taken in 2009 May--June showed the Balmer lines
in emission as well as numerous emission lines of iron, which is typical of
luminous blue variables (LBVs) near the visual maximum. New observations
carried out in 2015 May--September detected significant changes in the
spectrum, indicating that the star became hotter. We found that these changes
are accompanied by significant brightness variability of MN44. In particular,
the I_c-band brightness decreased by \approx 1.6 mag during the last six years
and after reaching its minimum in 2015 June has started to increase. Using
archival data, we also found that the I_c-band brightness increased by \approx
3 mag in \approx 30 yr preceding our observations. MN44 therefore represents
the seventeenth known example of the Galactic bona fide LBVs. We detected a
nitrogen-rich knot to the northwest of the star, which might represent an
interstellar cloudlet interacting with the circumstellar shell. We discuss a
possible association between MN44 and the INTEGRAL transient source of hard
X-ray emission IGR J16327-4940, implying that MN44 might be either a
colliding-wind binary or a high-mass X-ray binary.
