The galaxy presents as an elliptical morphology with a high degree of smoothness. It exhibits a generally round shape, tending slightly towards a disc-like form. There is no prominent disk structure visible.  The light distribution within the galaxy is concentrated towards the center.  Its color suggests a stellar population dominated by older stars. There is no visual evidence of ongoing or recent major merger events, though subtle signs of minor disturbances cannot be ruled out.  The galaxy appears quiescent, with low rates of star formation.
