The galaxy presents as a somewhat featureless, centrally concentrated object with a subtle disk structure. It displays a smooth, elliptical-like morphology with a gradual decrease in brightness from the core to the outer regions. No distinct spiral arms or bars are discernible. There is a faint bluish hue in the central region, perhaps suggestive of some degree of ongoing star formation, but it does not appear very vigorous. Overall the galaxy appears to be relatively undisturbed, although there may be slight distortions in the outer regions hinting at minor gravitational interactions.
