Image from Will Kinney@WKCosmo
Image is of an Analemma
The shape of the Analemma is due to change of declination and the equation of time.
The north–south component of the analemma results from the change in the Sun’s declination due to the tilt of Earth’s axis of rotation as it orbits around the Sun. The east–west component results from the nonuniform rate of change of the Sun’s right ascension, governed by the combined effects of Earth’s axial tilt and its orbital eccentricity.[1]
One can photograph an analemma by keeping a camera at a fixed location and orientation and taking multiple exposures throughout the year, always at the same time of day (disregarding daylight saving time).