The galaxy presents as a single, relatively smooth and centrally concentrated object. Its morphology appears largely elliptical or spheroidal, lacking any discernible spiral arms or a prominent disk. The light profile suggests a high degree of radial symmetry.

The galaxy's core exhibits a bright, concentrated emission, possibly indicative of an active galactic nucleus or a high density of stars. The color gradient transitions gradually from a yellower core to slightly bluer outer regions, suggesting ongoing star formation in the outskirts while the center is populated with older stellar populations.

There are no obvious signs of major mergers or significant tidal disturbances that would indicate recent interactions. The absence of clear dust lanes, distinct clumps of star formation, or strong asymmetries supports the classification of this galaxy as a relatively relaxed system.

Given the smooth structure and color gradient, it seems to be a massive galaxy, with a mass between 10^10 and 10^11 solar masses. Based on the data, it appears to be moderately star-forming for its type. The light is consistent with a redshift of approximately 0.22. 
