I will showcase the computation of the next-to-leading order scattering waveform using amplitudes. I will first give a brief overview of how to compute classical observables in gravity using scattering amplitudes in the KMOC formalism. I will then give an overview of the computation of the waveform, which corresponds to the 1-loop 5-point amplitude in gravity, with some numeric plots of the final result. I will conclude with a discussion of different aspects of the waveform, such as the memory effect and an IR divergent phase, along with future directions.