  We monitor the inner coma of comet 41P/Tuttle-Giacobini-Kres\'{a}k searching
for variations of its colour. Fast changes in colour of the comet
41P/Tuttle-Giacobini-Kres\'{a}k provide important clues for better
understanding of the microphysical properties of its dust. Using the 61-cm and
70-cm telescopes we measured the apparent magnitude of the comet with the V and
R Johnson-Cousins filters from January 29 until April 25 of 2017. The inner
coma ({\sim} 2000 km) reveals fast and significant variations of colour. The
most significant change was found between March 3 and 4 of 2017, when it
changed from blue with a colour slope S {\approx}(-10.15 {\pm} 3.43){\%} per
0.1 {\mu}m to red with S {\approx} (16.48 {\pm} 4.27){\%} per 0.1 {\mu}m. This
finding appears in good accordance with what was previously reported by Ivanova
et al. (2017) for long-period comet C/2013 UQ4 (Catalina), suggesting that fast
and significant variations of colour of dust could be a common feature of
short- and long-period comets. We model observations of comet
41P/Tuttle-Giacobini-Kres\'{a}k using the agglomerated debris particles and
conclude that its inner coma consists of a mixture of at least two types of
particles made of Mg-rich silicates and organics or Mg-Fe silicates.
