The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge.  The light distribution appears fairly even, fading gradually from a brighter core region, with no prominent spiral arm structures or significant dust lanes visible. The color index, based on the observed magnitudes, suggests a slightly bluer hue, indicative of ongoing, although potentially modest, star formation. Overall, the galaxy's structure seems relatively undisturbed, showing no strong signs of recent major merger events, although the possibility of minor gravitational disturbances cannot be ruled out. The object is roughly rounded in shape, with a slight deviation from perfect circularity.
