The galaxy presents as an elliptical or lenticular type, characterized by a relatively smooth, centrally concentrated light distribution. There is a pronounced bulge component that dominates the inner region, gradually fading into a more diffuse halo. The galaxy exhibits a mild ellipticity, with its longest axis extending approximately twice the length of its shortest. No distinct spiral arm structures or prominent dust lanes are discernible within the observed light distribution. The color profile appears generally uniform across the galaxy, showing a subtle gradient from a yellowish-white core to a slightly bluer outer halo. This color variation could indicate differing stellar populations, with older, redder stars concentrated in the core and younger, bluer stars populating the halo.
