  Optical broad-band spectral shape measurements of gamma-ray bursts (GRBs) are
typically made starting an hour or more after the trigger event. With our
automated, rapid-response system, the Burst Simultaneous Three-channel Imager
(BSTI) on the Nazarbayev University Transient Telescope at Assy-Turgen
Astrophysical Observatory (NUTTelA-TAO), we began measurements of GRB200925B
129 s after the Swift BAT trigger. The temporal decay log slopes in the g', r',
and i' bands in the time interval 129 s to 1029 s are -0.43 \pm 0.31, -0.43 \pm
0.15, and -0.72 \pm 0.14, respectively. During the decay phase, a shift in
color from red to blue, a change in log slope of \{beta} from -2.73 to -1.52
was measured. The evolution in the optical spectral slope is consistent with a
decrease in extinction caused by dust destruction.
