  Since its discovery in 1992, GRS 1915+105 has been among the brightest
sources in the X-ray sky. However, in early 2018, it dimmed significantly and
has stayed in this faint state ever since. We report on AstroSat and NuSTAR
observation of GRS 1915+105 in its unusual low/hard state during 2019 May. We
performed time-resolved spectroscopy of the X-ray flares observed in this state
and found that the spectra can be fitted well using highly ionised absorption
models. We further show that the spectra can also be fitted using a highly
relativistic reflection dominated model, where for the lamp post geometry, the
X-ray emitting source is always very close to the central black hole. For both
interpretations, the flare can be attributed to a change in the intrinsic flux,
rather than dramatic variation in the absorption or geometry. These reflection
dominated spectra are very similar to the reflection dominated spectra reported
for Active Galactic Nuclei in their low flux states.
