The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The light profile suggests an older stellar population, given the yellowish hue dominant in the central regions. There is little to no evidence of spiral arm structures or significant dust lanes within the galaxy. The overall appearance is largely undisturbed, indicating a lack of recent major merger events. There may be some minor asymmetry in the outer halo, but it is not definitive from this image alone.
