The galaxy presents as a smooth, elliptical form with a high degree of central concentration. Its overall shape is elongated, with the major axis significantly longer than the minor axis. The light profile appears to be centrally bright, with a gradual decline in surface brightness moving outwards. The galaxy exhibits a yellowish-white hue, suggesting an older stellar population. There is little indication of spiral arms or significant dust lanes, and no bright star-forming regions are discernible within the visible spectrum. The structure suggests that it has completed the majority of its star formation. There is no evidence of an ongoing merger or tidal disturbance.