early-time spectra, we detect $\lambda$5876 and P-Cygni profiles of [H$\alpha$]{} (with the absorption component greatly dominating over the emission component). The observation from 2001 Dec. 13, for example, shows the feature blueshifted by [$\sim\!\!$ ]{}16,000 [km s$^{-1}$]{}. In addition, @Phillips01 mention that there are broad absorption features at 4080 Å and 4580 Å in the observation from 2001 Dec. 13, and it is possible that they are [H$\gamma$]{} and [H$\beta$]{}, respectively. However, the observation lacked acceptable blue-side flatfields and proper wavelength-calibration files, so data at wavelengths $\lesssim$5000 Å cannot be completely trusted. We also identify the very weak, broad absorption near 7300 Å as $\lambda$7774. By 13 days after the explosion many more spectral features have appeared. Still present are the P-Cygni profile of [H$\alpha$]{}  and the $\lambda$5876 line. @Maund07 point out that [H$\alpha$]{} at this time is likely to be blended with $\lambda$6678. No longer visible in this spectrum is the aforementioned “W” feature that probably came from a combination of , , and . This is again similar to SN 2008D, whose “W” disappeared in the span of [$\sim\!\!$ ]{}1 day [@Modjaz09]. However, there [*are*]{} still features at about 4130 Å and 4287 Å, and we associate these 