The galaxy appears to be an elongated elliptical shape, possibly a prolate spheroid viewed at an angle. The light distribution suggests a smooth profile, with a concentration of older stars, as indicated by the yellowish-red hue of the central region. The edges are less defined, appearing to fade out gradually into the background, suggesting an extended halo or envelope. There might be subtle signs of tidal disturbances, as evidenced by asymmetry and potential faint tails, which could indicate an interaction or merger history. The object displays negligible recent or ongoing star formation within the observable spectra. The estimated size would place it among the larger galaxies within its redshift. 
