The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated bulge. The core exhibits a bright, yellowish-white hue. The outer regions display a fainter, more reddish tint, suggesting an older stellar population. There is a smooth gradient in brightness, diminishing from the core outwards. No prominent spiral arms or disk features are discernible. There are no signs of tidal tails or major disturbances, suggesting it is not currently undergoing a major merger event.
