The galaxy appears as a centrally concentrated, relatively smooth structure with a generally elliptical morphology. The core of the galaxy exhibits a bright, yellowish-white hue, suggesting an older stellar population. Moving outward from the core, a faint, diffuse halo is observed, displaying a subtle greenish-blue tint. There is no discernable spiral arm structure or obvious dust lane features in this image. The overall appearance is consistent with that of an elliptical galaxy, or possibly a lenticular galaxy viewed at a shallow inclination. There is some slight unevenness in the outer regions but nothing to suggest that it is undergoing a major merger.
