The galaxy presents as a smooth, elliptical structure. Its overall form is highly regular and round, with no obvious signs of a disk-like morphology. There is a color gradient moving outward from the center of the galaxy indicating a possible change in stellar population and the presence of dust or gas. No significant morphological distortions or tidal features are visible, suggesting it is not currently undergoing a major merger event. The central region appears quite bright, with brightness generally decreasing towards its outer regions.
