The galaxy presents as an elliptical or lenticular type object. It exhibits a generally smooth morphology, with a high degree of central concentration. The core region displays a yellowish hue. The isophotes appear moderately elliptical, with a noticeable elongation along one axis. A subtle color gradient suggests potential variation in stellar populations or dust distribution within the galaxy. There is no strong evidence of prominent spiral arms or a well-defined disk structure. No significant tidal features or obvious signs of recent merger activity are apparent. The overall structure indicates a relatively evolved system. 
