The galaxy appears to be a relatively compact system. The overall morphology is smooth and elliptical, with a high degree of central concentration of light. There is a subtle color gradient, with the core region exhibiting a more yellowish-white hue and the outer regions gradually becoming slightly bluer. There is no apparent spiral structure or prominent disk component. The overall light profile suggests a lack of significant ongoing star formation. Indications of minor disturbances are visible, though there are no signs of an ongoing merger, nor of major disruptions to the overall shape. 
