The galaxy presents a largely smooth, elliptical morphology. It appears concentrated with a gradual decrease in surface brightness from its center. The color gradient indicates a predominantly older stellar population, with a yellowish hue suggesting the presence of evolved stars. The galaxy exhibits a subtle deviation from perfect sphericity, leaning towards a more oblate shape. There are no clear signs of spiral arms or significant dust lanes visible in this image. The object displays no obvious signs of ongoing major merger activity, however, some minor tidal disturbances may be occurring. Its light output suggests it to be a fairly luminous object. Overall, this appears to be a relatively quiescent, massive galaxy with a low star formation rate.
