  2I/Borisov is the first-ever observed interstellar comet (and the second
detected interstellar object). It was discovered on 30 August 2019 and has a
heliocentric orbital eccentricity of ~ 3.35, corresponding to a hyperbolic
orbit that is unbound to the Sun. Given that it is an interstellar object, it
is of interest to compare its properties -- such as composition and activity --
with the comets in our Solar System. This study reports low-resolution optical
spectra of 2I/Borisov. The spectra were obtained by the MDM observatory Hiltner
2.4m telescope/Ohio State Multi-Object Spectrograph (on 1 and 5 November 2019).
The wavelength coverage spanned from 3700A to 9200A. The dust continuum
reflectance spectra of 2I/Borisov show that the spectral slope is stepper in
the blue end of the spectrum (compared to the red). The spectra of 2I/Borisov
clearly show CN emission at 3880A, as well as C2 emission at both 4750A and
5150A. Using a Haser model to covert the observed fluxes into estimates for the
molecular production rates, we find Q(CN) = 2.4 +/- 0.2 x 10^24 s^-1, and Q(C2)
= 5.5 +/- 0.4 x 10^23 s^-1 at the heliocentric distance of 2.145 au. Our Q(CN)
estimate is consistent with contemporaneous observations, and the Q(C2)
estimate is generally below the upper limits of previous studies. We derived
the ratio Q(C2)/Q(CN) = 0.2 +/- 0.1, which indicates that 2I/Borisov is
depleted in carbon chain species, but is not empty. This feature is not rare
for the comets in our Solar System, especially in the class of Jupiter Family
Comets.
