The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated bulge with a noticeable radial decrease in surface brightness. The core region is quite luminous, appearing almost spheroidal. The color profile suggests a population of older stars, trending toward redder hues, particularly in the central region, with a subtle shift towards bluer tones in the outer regions. No distinct spiral arms or prominent dust lanes are visible. There are no obvious signs of active galactic nuclei activity, although this cannot be definitively determined from the image alone. Overall, the galaxy presents as a relatively undisturbed system with a high degree of symmetry.
