The galaxy presents a generally smooth morphology. It appears elliptical in shape, displaying a high degree of roundness. The color profile suggests an older stellar population, with a yellow-orange hue dominating the central region, indicating the presence of evolved stars. No distinct spiral arms or prominent dust lanes are apparent. There is a slight color gradient from the core outwards, with the outer regions appearing less luminous and slightly redder than the central bulge. There's no obvious evidence of ongoing mergers or major disturbances within the galaxy's structure, with only some very faint possible disturbances.
