Its semi-major axis of 0.7237 AU is very similar to that of Venus, but its eccentricity is relatively large (0.4104), and its orbital inclination is also significant (9.0060°).

Its rotational period is 13.5 hours, and its light curve has an amplitude of 0.9 mag, which hints at a very elongated body, perhaps a contact binary.

Zoozve was identified as a quasi-satellite of Venus by Seppo Mikkola, Ramon Brasser, Paul A. Wiegert and Kimmo Innanen in 2004, two years after the actual discovery of the object.

[5][6] From the perspective of a hypothetical observer in a frame of reference rotating with Venus, it appears to travel around the planet during one Venusian year.

Zoozve is included in the Minor Planet Center list of Potentially Hazardous Asteroids (PHAs) because it comes relatively frequently to within 0.05 AU of Earth.

[8] This led Skiff to propose the name "Zoozve", on Nasser's behalf, to the International Astronomical Union's Working Group Small Bodies Nomenclature (WGSBN).