We performed follow-up measurements of this object, while it was still on the neocp. Stacking of 18 R-filtered exposures, 30-sec each, obtained remotely, from the Haleakala-Faulkes Telescope North on 2013, June 04.5, through a 2.0-m f/10.0 Ritchey-Chretien + CCD (operated by Las Cumbres Observatory Global Telescope Network), shows that this object is a comet: sharp central condensation, surrounded by a faint coma nearly 4" in diameter.
M.P.E.C. 2013-L41 assigns the following preliminary parabolic orbital elements to comet C/2013 L2: T 2012 Apr. 29.80; e= 1.0; Peri. = 359.60; q = 4.77; Incl.= 106.44
by Ernesto Guido & Nick Howes