The galaxy presents a largely smooth and elliptical morphology. It exhibits a central concentration of light that diminishes gradually towards its outer edges. The core appears yellowish-white, possibly indicating an older stellar population. Faint blue tinges may be indicative of some present star formation but are mostly overwhelmed by an older population. There are some apparent very minor structural irregularities in the outer regions of the disk, which could suggest either a slight disturbance or perhaps a minor merger event at some point. The observed axial ratio suggests it is not perfectly spherical but rather somewhat elongated. The object appears to be a relatively large and massive system.
