 In the SMASS classification, "Pawlowia" is a K-type asteroid, which are common among members of the Eos family and known for their intermediate albedo.In September 2003, a tentative rotational lightcurve of "Pawlowia" was obtained from photometric observations by American Maurice Clark at the Bucknell and Rosemary Hill Observatory in Pennsylvania and Florida, respectively.Analysis of the essentially flat lightcurve gave a poorly rated rotation period of 8.23 hours with a brightness amplitude of at least 0.02 magnitude ().