The galaxy presents a generally smooth, elliptical morphology with a high degree of circularity. There is no discernible disk structure or spiral arm features evident in the image. The galaxy's core region appears bright and concentrated, suggesting a potentially high stellar density. A slight color gradient is observed, transitioning from a whiter central region to a slightly greener outer halo. There are no obvious signs of major mergers or tidal disturbances. The galaxy appears relatively isolated and undisturbed within its immediate environment.
