This galaxy presents as an elliptical galaxy with a smooth, diffuse morphology and a high degree of central concentration. There is a noticeable yellowish-white hue at the core, which likely indicates an older stellar population. The outer regions appear to fade gradually into the background, with a slight suggestion of a faint, flattened disk-like structure oriented horizontally to the image. No distinct spiral arms or dust lanes are readily visible, but there is a hint of a feature or disruption on the right side of the image. Overall, this galaxy exhibits characteristics consistent with a passive, evolved system.
