The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a concentrated brightness, transitioning outward to a more diffuse halo. The light distribution suggests a moderate degree of flattening. There is a slight colour gradient noticeable, shifting from a yellowish core to a bluer outer region. Weak indications of a faint spiral structure are present, though not clearly defined. There are hints of some minor disturbances, which could possibly be interactions with small satellite galaxies. 
