Spectroscopic follow-up of SN 2013ej was primarily obtained using the twin FLOYDS spectrographs on FTS and the Faulkes Telescope North, at Haleakala, with an ~1d cadence. Optical spectra were also obtained at the Asiago 1.22m telescope with the B&C spectrograph. Optical (UBVRIgriz) photometric follow-up of SN 2013ej was obtained with the nine 1 m telescopes of the LCOGT network, and in this Letter we present data obtained up to one month after the SN discovery. (1 data file).