This project provides spectroscopic followup for the SS 433 candidates presented by Calzetti et al. (1995).  Each target object is cross-referenced with surveys of other sources and PHATTER F475W imaging.  A total of 40 of the 408 well-covered objects were classified as one of six types. None of the candidates meet the requirements to be considered an SS 433-like object. This result effectively rules out the presence of an SS 433 analog in M33.