The galaxy appears to be an elliptical galaxy, exhibiting a smooth and concentrated light profile. Its overall shape is largely spheroidal, deviating minimally from perfect circularity. The central region displays a significantly higher surface brightness compared to the outer regions, indicating a concentration of stars and possibly a supermassive black hole at the galactic nucleus. There is little indication of spiral arms or significant dust lanes. The color of the galaxy is predominantly yellowish-white, suggesting an older stellar population with a lower rate of star formation. There is some mottling in the outskirts, possibly indicating some tidal debris or faint outer star clusters. No signs of a major ongoing merger are immediately apparent, but the presence of minor disturbances cannot be ruled out based on this image alone.
