The galaxy presents a smooth, largely featureless morphology, appearing elliptical in shape, with a high degree of central concentration. The light distribution suggests a near-spherical form, with minor deviation. Color gradients indicate a concentration of older stellar populations in the core region, appearing more yellow, while bluer hues are diffused in the outer halo. No significant signs of dust lanes, spiral arms, or tidal features are visible. This morphology suggests a quiescent galaxy with negligible ongoing major star formation activity, and no signs of recent or ongoing mergers or major disturbances.