It was observed for only one month between September 24 and October 26
in 1960. It has not been observed since that.
Because of the large perihelion distance of 4 A.U., it returns almost
in the same condition every time. It is always faint.
The previous return was in 1994, when LINEAR or NEAT have not surveyed
yet.
In 2011, it will return in the era of automated survey for the first
time. So it may be recovered.