The galaxy presents a predominantly smooth morphology, with an ellipsoidal shape. The light distribution appears centrally concentrated, fading gradually towards the outer regions. The core exhibits a bright, yellowish hue, potentially indicating an older stellar population. There is a subtle transition in color towards the outer edges, with a slight shift towards redder tones. There are no obvious signs of spiral arm structures or significant dust lanes within the galaxy. Overall, this galaxy appears to be a relatively undisturbed system, showing no strong evidence of recent major merger events.
