The galaxy presents as a single, relatively smooth, and luminous entity. Its morphology appears predominantly elliptical. There is a high concentration of light towards the center, suggesting a prominent galactic nucleus or bulge. The light from the galaxy is generally yellow-red, with this color concentrated at the center. The outer regions of the galaxy exhibit a gradual decrease in luminosity, with no apparent substructure or distinct spiral arms visible. Overall the galaxy has a very round appearance. There is no visible evidence of significant tidal disturbances or ongoing mergers. Given the galaxy's smooth appearance, redshift, and color indices, it is plausible that star formation is suppressed.
