The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth overall appearance. The light profile indicates a gradual decrease in brightness outwards from the core. The central region exhibits a yellowish hue, suggestive of an older stellar population. There's a subtle extension or slight asymmetry apparent, hinting at a possible past interaction or minor disturbance in its morphological structure. No distinct spiral arms or significant dust lanes are discernible within the galaxy's disk. The object is relatively compact, with a moderate angular size.
