  We report multiband observations of the Optical Transient (OT) associated
with GRB000301c carried out between 2--4 March 2000 using the 2.34-m Vainu
Bappu Telescope (VBT) at Kavalur, India. When combined with other reported
data, the initial decline in the R-band magnitude with log ($t-t_0$), the time
since the burst is fit with a slope $\alpha_{1}$ = -0.70 $\pm$ 0.07 which
steepens after about 6.0 days to a slope of $\alpha_{2}$ = -2.44 $\pm$ 0.29.
This change in slope does not occur smoothly but there is an indication for a
bimodal distribution. The available measurements of the evolution of (B--R)
color do not show any discernible evolution in the first 12 days.
