The galaxy presents as a relatively smooth, elliptical-like structure. The core appears concentrated and bright, emitting a yellowish-white light, potentially indicating an older stellar population. The light intensity decreases gradually from the center outwards, forming a halo. There is faint color variation in the outer regions, with hints of bluer hues, possibly indicative of younger stars forming at a low rate. There is no sign of spiral arms or a bar. No major merger events or significant disturbances are apparent in this image. The galaxy exhibits a high degree of roundness.
