The galaxy presents as an elliptical or lenticular type. It exhibits a dominant, centrally concentrated bulge. The bulge displays a smooth, yellowish-white color suggesting an older stellar population, with little evidence of ongoing star formation. The galaxy's outer regions show a gradual decrease in brightness. The overall structure appears relatively undisturbed, with no signs of major mergers or tidal interactions. The visible light is somewhat redder than the light from younger galaxies, possibly indicating substantial dust content or a lack of young, blue stars. The galaxy is not perfectly round but has a slight elongation. No distinct spiral arms or other features can be discerned in the image, implying a relatively smooth and featureless morphology.
