  We present a detailed spectroscopic analysis of the recently discovered fast
evolving Type I superluminous supernova (SLSN-I), SN 2019neq (at redshift z =
0.1059) comparing it to the well-studied slow evolving SLSN-I, SN 2010kd (z =
0.101). Our investigation concentrates on optical spectra taken during the
photospheric phase. The observations of SN 2019neq were carried out with the
10m Hobby-Eberly Telescope (HET) Low Resolution Spectrograph-2 (LRS2) at
McDonald Observatory. We apply the SYN++ code to model the spectra taken at -4
days, +5 days and +29 days from maximum light. We examine the chemical
evolution and ejecta composition of the SLSN by identifying the elements and
ionization states in its spectra. Our analysis confirms that SN 2019neq is a
fast evolving SLSN-I. We derive the number density of each ionization state at
the epoch of the three observations. Finally, we give constraints on the lower
limit of the ejecta mass and find a hint for a possible relation between the
evolution timescale and the ejected mass of SLSNe-I.
