The galaxy appears to be elliptical in shape. It shows a smooth and centrally concentrated luminosity profile, with a gradual decrease in brightness from the core outwards. There's a noticeable elongation, creating an oval appearance. The overall color suggests a population of older stars, with a subtle bluish tint near the center and a shift towards redder hues in the outer regions. There is no apparent disk structure or spiral arms. The galaxy appears isolated, with no obvious signs of recent or ongoing mergers or interactions.
