Observed spectra of SMCSGS-FS 69 (blue solid lines) displaying narrow and broad components. The composite model (dashed red) is the weighted sum of the stripped star primary (dotted brown) and the rapidly rotating Be star secondary (dashed green) model spectra with effective temperatures of 24 kK and 28 kK, respectively. The weaker absorption core in Hγ likely results from filled-in disk emission.