The galaxy presents as a relatively smooth, centrally concentrated object. It appears mostly elliptical in shape, with a minor deviation toward a slightly oblong form. There's a gradual decrease in luminosity from the core outwards, with no discernible spiral arm structures or significant dust lanes. The color profile suggests a relatively homogenous stellar population, possibly dominated by older stars, showing a hue shift towards redder wavelengths. It seems largely undisturbed.
