The galaxy presents as a largely featureless elliptical or lenticular morphology. It is generally smooth in appearance, with a bright, concentrated central bulge. The light distribution decreases gradually away from the core. There is a subtle color gradient visible from the center outwards, trending slightly redder at the core and subtly bluer towards the edge. No distinct spiral arms or dust lanes are evident. The overall shape is neither perfectly round nor particularly elongated. There is a hint of disturbance or asymmetry in the outer regions, although no clear signs of a major ongoing merger are obvious in the image. The overall red color suggests an older stellar population and a lower star formation rate.
