  We present temporal and time-integrated spectral analyses of 148 bursts from
the latest activation of SGR J1935+2154, observed with Fermi/GBM from October
4th 2019 through May 20th 2020, excluding a ~130 s segment with a very high
burst density on April 27th 2020. The 148 bursts presented here, are slightly
longer and softer than bursts from earlier activations of SGR J1935+2154, as
well as from other magnetars. The long-term spectral evolution trend is
interpreted as being associated with an increase in the average plasma loading
of the magnetosphere during bursts. We also find a trend of increased burst
activity from SGR J1935+2154 since its discovery in 2014. Finally, we find no
association of typical radio bursts with X-ray bursts from the source; this
contrasts the association of FRB 200428 with an SGR J1935+2154 X-ray burst, to
date unique among the magnetar population.
