The galaxy appears as a somewhat diffuse, elliptical-shaped object with a centrally concentrated bulge. There is a subtle elongation noticeable, but it mostly appears between round and elliptical. The central region exhibits a yellowish-orange hue, potentially indicating an older stellar population. Fainter, bluish extensions emanate from the main body, possibly representing regions of younger star formation. One such extension is larger and appears to be separated from the galaxy body. The galaxy does not present a smooth morphology; some minor disturbances can be seen. The overall structure suggests an evolved system with ongoing, but potentially limited, star formation.
