The galaxy presents as an elliptical-type morphology, with a generally smooth light distribution. The core is bright and concentrated, fading gradually towards the outer regions. Color gradients are subtle, but a slight reddening may be present towards the center compared to the slightly bluer fringes of its halo. No distinct spiral arms or dust lanes are observed. The galaxy's shape is neither perfectly spherical nor significantly elongated, appearing to have an intermediate ellipticity. No signs of any major ongoing merger events are visually apparent, though there is some minor visible disturbance.
