The galaxy presents a generally smooth morphology. It appears elliptical in shape, exhibiting a high degree of central concentration with a bright, yellowish core. The color gradient suggests an aging stellar population with relatively little active star formation, consistent with the smooth morphology and lack of prominent spiral arms or dust lanes. There are no obvious signs of tidal disturbances or ongoing mergers, indicating that the galaxy has likely evolved in relative isolation or completed any past mergers. The isophotes appear largely regular, with only slight deviations from perfect ellipticity, suggesting a well-mixed stellar population and a dynamically relaxed system. 
