In the past, one could view a 3D visualization of the body's orbit using a Java applet. As of mid-2023, one could see something similar using JPL's Orbit Viewer tool, which was implemented using JavaScript, Three.js and WebGL.
The orbit viewer uses unreliable two-body methods, and hence should not be used for accurately determining the time of perihelion passage or planetary encounter circumstances. For accurate ephemerides use the JPL Horizons On-Line Ephemeris System that handles the n-body problem using numerical integration.4
"Small-Body Database Lookup". ssd.jpl.nasa.gov. Retrieved 2021-10-01. https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/ ↩
"JPL Small-Body Database browser". NASA/JPL. Archived from the original on 2021-09-22. Retrieved 2012-03-19. https://ssd.jpl.nasa.gov/sbdb.cgi ↩
"Solar System Objects at JPL Solar System Dynamics". Archived from the original on 2021-09-19. Retrieved 2021-09-27. https://ssd.jpl.nasa.gov/ ↩
JPL Note https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=54509621&view=V ↩