The galaxy appears to be a relatively smooth, elliptical or lenticular system. The central region exhibits a high degree of luminosity, fading gradually towards the outer edges. The overall color profile suggests a population of older stars, with a yellowish hue dominating the central bulge. A slightly off-center region displays a feature suggestive of ongoing star formation, exhibiting a bluer color. The isophotes appear mostly regular, although there is a subtle asymmetry hinting at a possible minor interaction or past merger event. No prominent spiral arms or dust lanes are clearly visible. The galaxy's general form indicates a later-type system, relatively evolved and potentially transitioning toward a more quiescent state.
