GRB 971214 Optical Observations #013 S. G. Djorgovski, S. R. Kulkarni, J. S. Bloom (Caltech), R. Goodrich (WMKO), and D. A. Frail (NRAO) report on behalf of the Caltech GRB collaboration: "Analysis of the spectra of the proposed optical transient counterpart (OT) of GRB 971214, obtained at the Keck-II 10-m telescope on 17 Dec 1997 UT, shows a possible detection of an extended emission line at a wavelength of 7567 A. It is also intriguing that a faint emission line at a similar wavelength (7533 A) has been detected from a faint galaxy about 4.5 arcsec north of the OT (see our previous email on GCN3). If this line emission from the OT is real, it can be interpreted as the [O II] 3727 line at z = 1.03. However, we emphasize that this marginal detection has to be checked with additional data."