The galaxy presents a smooth, elliptical morphology. Its light profile appears highly concentrated towards the center, suggesting a dominant bulge component. The galaxy exhibits a gradual decrease in surface brightness moving outward from the core with a relatively round shape. Color gradients are subtle, with the central region appearing slightly yellower compared to the outer regions, which have a somewhat redder hue. No distinct spiral arms or prominent dust lanes are discernible in this image. The overall appearance indicates a relatively evolved system with a moderate stellar mass. There does not appear to be evidence of ongoing major mergers or significant tidal disturbances.
