The galaxy presents an overall elliptical morphology. Its shape appears somewhat flattened or elongated, not perfectly circular. The galaxy exhibits a smooth, centrally concentrated light distribution, with a gradual decrease in intensity from the core outwards. The central region presents a bright, yellowish hue, indicative of an older stellar population. The outer regions are fainter and display a slightly bluer color, suggesting the presence of younger stars. There is no evidence of distinct spiral arms, dust lanes, or other features associated with disk galaxies. The galaxy appears relatively undisturbed, showing no signs of recent mergers or interactions.
