The galaxy exhibits a centrally concentrated morphology with a smooth appearance, suggesting it is likely an elliptical galaxy or a lenticular galaxy viewed face-on. The core is bright and yellowish-white, indicating an older stellar population. There is a gradual decrease in brightness moving outward from the core to the surrounding halo. The galaxy is generally rounded in shape, with no obvious signs of strong spiral arms or a bar structure. Faint blueish and reddish tinges are present in the outskirts, which may indicate regions of younger star formation. There is no evidence of major ongoing mergers or significant tidal disturbances, though subtle irregularities in the outer halo cannot be ruled out. Based on its size and absolute magnitude, this galaxy is likely a massive galaxy. 
