The galaxy appears to be an elliptical or lenticular type, displaying a smooth, featureless morphology. It is roughly circular, exhibiting minimal deviation from a perfect sphere, with a slight elongation. The color profile suggests an older stellar population, with a dominant yellowish-red hue in the central bulge, fading into a slightly bluer periphery. There's no distinct evidence of spiral arms or dust lanes within the visible light spectrum. Slight disturbances in the outer regions cannot be ruled out, though this could also be effects of image resolution limitations. No apparent signs of ongoing major merger events are discernible, however there might be minor interactions occurring.
