The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be mostly featureless, showing a centrally concentrated light profile with a gradual decrease in intensity towards the outer regions. There is a slight elongation visible, with the galaxy not appearing perfectly circular. The color profile suggests a dominant older stellar population, indicated by the reddish-yellow hue concentrated towards the center, fading into a bluer halo in the outskirts. No distinct spiral arms, bar structures, or significant dust lanes are discernible. There may be some evidence of minor interaction or disturbance, though the overall structure seems largely undisturbed.
