New photoelectric UBV photometry in the open cluster NGC 5460 is prese
nted for 155 stars brighter than 14.0 mag. In addition, six comparativ
ely bright red stars in the cluster field were observed in the DDO and
Washington systems. Nearly 40% of the observed stars are found to be
members or probable members. The analysis of the new data yields E(B -
V) = 0.12 +/- 0.03 and V0 - M(v) = 9.34 +/- 0.20 (740 +/- 68 pc) for
the cluster reddening and true distance modulus, respectively. An age
of 1.1 10(8) yr was derived, which places this cluster within the NGC
2516 age group. NGC 5460 does not probably contain any red giant.