The galaxy presents as a singular, relatively symmetrical structure. Its overall morphology appears smooth and elliptical, with a high degree of circularity. The light is centrally concentrated, displaying a bright, well-defined core that gradually diminishes in intensity toward the outer edges. There is little evidence of spiral arms, bars, or other distinct features typically associated with disk galaxies. No obvious signs of ongoing merging activity or tidal disturbances, like extended plumes or distortions, are visible. The galaxy appears to be a fairly well-formed spheroid galaxy. A color gradient is observed, shifting from yellow at the center to red at the periphery. This could indicate an aging stellar population with suppressed star formation.
