The galaxy appears as a relatively smooth, elliptical-shaped structure. There is a slight elongation, but it is generally round. The central region exhibits a brighter, yellowish hue, suggesting a concentration of older stars. The outer regions fade gradually, indicative of a decreasing stellar density. No distinct spiral arms or dust lanes are visible. There is some possibility of minor disturbances present but no definite indication of recent or ongoing major merger activity. The overall morphology suggests this is likely a massive galaxy with a relatively low rate of star formation.
