The galaxy presents as a relatively smooth, elliptical structure. Its overall shape appears round, exhibiting minimal deviations from circular symmetry. A luminosity gradient is observed, with the central region displaying the highest surface brightness, gradually decreasing towards the outer edges. No distinct features, such as spiral arms, bars, or dust lanes, are discernible within the galaxy's morphology. The galaxy exhibits a yellowish hue, suggestive of an older stellar population dominating its composition. There is no indication of ongoing major merger events or significant tidal disturbances, although the possibility of minor interactions cannot be ruled out based on this single image.
