The galaxy appears to be a relatively compact and luminous object at a redshift of approximately 0.19. Morphologically, it presents as a smooth or elliptical galaxy, lacking distinct spiral arms or a prominent disk structure. It is more elongated than circular. No signs of strong tidal disturbances or ongoing major mergers are apparent in this image, though there may be some indications of a minor disturbance. The galaxy exhibits a stellar mass around 10^10.7 solar masses, placing it in the category of a massive galaxy. The specific star formation rate is estimated to be quite low, suggesting a relatively quiescent phase of stellar evolution. The galaxy exhibits an absolute magnitude in the g-band around -21. The half-light radius is around 5 kpc.
