The galaxy appears to be a relatively smooth, elliptical-like structure, characterized by a centrally concentrated spheroid. The core region exhibits a bright, diffuse glow, suggesting a high density of stars. The light profile gradually diminishes outwards from the core, transitioning into a fainter halo. There are no easily discernable spiral arms or distinct morphological features. A slight elongation is observable, but the galaxy is generally rounded in appearance. Faint hints of possible minor disturbances or tidal features are present in the outer regions, though the resolution limits definitive confirmation. The color gradients within the galaxy may indicate variations in stellar populations or dust content, with the central region appearing somewhat redder than the outer regions. Overall, the galaxy seems to be an evolved system, possibly undergoing a period of quiescence in its star formation activity.
