In theSMASS-I taxonomy, this is classified as anS-type asteroid.[3] It spans a girth of approximately 50 km.[1] The rotation of this asteroid is commensurate with the length of an Earth day, requiring measurements from more than one latitude for full coverage.Photometric observations from the US and Australia in 2012 provided an estimatedrotation period of25.107±0.005 h with a brightness variation of0.16±0.02 in magnitude. This is consistent with the results of an earlier study in 2006.[4]
^Oey, Julian; et al. (April 2013), "Lightcurve Analsyis of 774 Armor and 3161 Beadell",Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers,40 (2): 64,Bibcode:2013MPBu...40...64O.