The galaxy presents as a centrally concentrated, moderately luminous object at a redshift of approximately 0.21. Morphologically, it appears largely smooth and elliptical in shape, showing a gradual decrease in surface brightness from the center outwards, with no readily discernible spiral arms or bar structures. The galaxy appears to be somewhat rounded but not perfectly so, with a hint of elongation in its overall structure. A subtle color gradient is observed, with the core exhibiting a yellowish-white hue, suggestive of an older stellar population, while the outer regions show a slightly bluer tint, potentially indicating the presence of some younger stars or ongoing low-level star formation. There is no strong evidence of significant tidal disturbances or recent major merger activity.
