The galaxy presents as a singular, concentrated luminous body with a smooth, elliptical morphology. The primary light emission is characterized by a yellowish-golden hue, suggesting an older stellar population with minimal ongoing star formation. The galaxy exhibits a high degree of central concentration. There is a slight suggestion of a faint, diffuse halo extending outwards, though its boundaries are poorly defined. There is no visible evidence of spiral arms, bars, or significant dust lanes. There are no signs of any major interactions or disturbances in the shape of the galaxy.
