The galaxy appears to be an elliptical galaxy. It presents as a single smooth object, with no obvious spiral arms or disk structure. The galaxy exhibits a centrally concentrated luminosity profile, gradually decreasing in intensity towards the outer edges. The core region appears yellow, potentially indicating an older stellar population. The outer regions display a slightly bluer hue, which may signify the presence of some younger stars, or a lower concentration of dust, but the galaxy as a whole does not present signs of substantial recent star formation. The shape is mostly round. There is no evidence of any ongoing merger activity or tidal disturbances, although there is very minor, slight distortion in the shape of the outer halo.
