The galaxy presents a generally smooth morphology, appearing elliptical in shape. It exhibits a noticeable color gradient, transitioning from a yellowish core to slightly redder hues in its outer regions. The central bulge is prominent and relatively bright, suggesting a high concentration of stars. The overall structure lacks prominent features such as spiral arms or dust lanes. A slight elongation is visible, potentially indicating a mild degree of rotational support or a triaxial structure. There is no immediately apparent evidence of ongoing major mergers or strong tidal interactions. However, the possibility of minor disturbances in its outer halo cannot be definitively ruled out based on this image alone.
