The galaxy presents as a relatively smooth, elliptical object. The light distribution is centrally concentrated, displaying a gradual decrease in intensity from the core outwards. There is a slight elongation, deviating from a perfectly circular shape, tending towards an elliptical form. There is no indication of spiral arm structures or dust lanes. The color appears generally uniform across the galaxy's body, with a slight shift towards redder hues indicating an older stellar population. There does not appear to be any major disturbances or ongoing merger events, although a minor asymmetry in the outer regions could be interpreted as the remnants of a previous interaction.
