The galaxy presents as a relatively compact structure with a general morphology that appears to be elliptical or lenticular. It exhibits a smooth light distribution overall, with no prominent spiral arms or obvious bar structure visible. There are some faint disturbances, suggesting a possibility of minor mergers. The galaxy presents a light blue hue, indicating the presence of young stars. The apparent size is small, indicating that it is a galaxy observed at significant cosmological distance. It would be beneficial to investigate if its spectra match that of a relatively young and compact galaxy.
