The galaxy exhibits a relatively smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The central region shows a high concentration of light, suggesting a prominent galactic nucleus or bulge. The galaxy displays a color gradient, with the central regions appearing more yellow or golden, while the outer regions appear slightly redder. This could indicate a difference in stellar populations, with older, redder stars dominating the outer regions and potentially younger, hotter stars or dust present in the inner regions. The overall shape suggests a high degree of symmetry, although it appears slightly elongated along one axis, implying a mild degree of ellipticity. There's no visible sign of ongoing major mergers or significant tidal disturbances in this image.
