The galaxy appears as a concentrated central bulge, exhibiting a smooth, elliptical morphology. There is a slight elongation, but it is generally round. The core region presents a bright, yellowish-white hue, suggesting an older stellar population. Fainter, bluer light surrounds the core, implying the existence of some younger stars within a disk structure that extends beyond the central bulge. No distinct spiral arms or bars are apparent. There are no signs of ongoing or recent major merger events.
