The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that is bright and appears yellowish-white in color, suggesting an older stellar population. The galaxy fades gradually outward from the center, indicating a decreasing density of stars and gas. There is subtle evidence of a disk-like structure. The color gradients suggest ongoing, although possibly low, levels of star formation within the disk. There is no apparent major disturbance to the overall structure and no indications of on-going merger activity.
