Subsequent study of CEERS 1019 involved measurement of nitrogen abundance relative to oxygen (a standard reference point for metallcitiy) using ultraviolet lines emitted by oxygen, O III] 1660, and nitrogen, N IV] 1486 and N III 1750. Other abundances, such as carbon (measured from C III] 1909) follow the trends anticipated from observations of nearby galaxies and from stellar nucleosynthesis models. However, CEERS 1019 exhibits an excess of nitrogen relative to oxygen. This extra nitrogen may be related to very massive stars unique to the early universe and related stellar winds (similar to Wolf-Rayet stars in the nearby universe) actively enriching the ISM. The excess nitrogen in CEERS 1019 is similar to that seen in GN-z11 and may be characteristic of galaxies in the early universe.