The galaxy presents as a relatively smooth, elliptical structure with a noticeable elongation. It displays a centrally concentrated bulge that appears to be the brightest region. There is a color gradient, with the core exhibiting a slightly redder hue compared to the outer regions, which show a tint that is slightly less red. No distinct spiral arms or dust lanes are readily apparent. There may be very minor irregularities or disturbances, but overall the morphology suggests a system that has largely settled into a more spheroidal shape.
