The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominating the central region. The galaxy's isophotes appear elongated, with a position angle oriented roughly northwest to southeast. The outer regions display a gradual decrease in surface brightness, transitioning into a reddish halo. There is no clear evidence of spiral arms or significant dust lanes within the image, reinforcing its classification as an elliptical galaxy. The overall color profile indicates a low star formation rate. There is no apparent merging or major disturbances in the structure.
