 According to the overall spectral type for members of the Eunomia family, "Meta" is an assumed S-type asteroid.In October 2006, a rotational lightcurve of "Meta" was obtained from photometric observations by French amateur astronomer René Roy.Lightcurve analysis gave a well-defined rotation period of 6.142 hours with a brightness amplitude of 0.46 magnitude, indicating that the asteroid has an elongated shape ().