The galaxy presents a largely smooth and centralized morphology. It exhibits a generally elliptical shape, appearing more "in between" than perfectly round or cigar-shaped. There is a dominant central bulge. No substantial spiral arm structure or distinct disk components are readily apparent. It has an apparent magnitude dim enough that it's only observed in the DESI bands. The galaxy exhibits moderate star formation activity, and a calculated mass that would classify it as a massive galaxy. No major merger events or significant tidal disturbances are obvious upon inspection.
