The galaxy presents a primarily elliptical morphology, exhibiting a smooth and relatively featureless structure. The central region displays a high concentration of light, appearing as a bright, yellowish core. The light intensity decreases gradually towards the outer edges of the galaxy, forming a diffuse halo. There is a subtle disk-like structure, but the overall morphology is dominated by the spheroid. Minor asymmetry is present, but no major disturbances or signs of ongoing merger events are readily apparent. There is negligible star formation. The galaxy appears to be an evolved system with primarily older stellar populations.
