The galaxy presents as a lenticular-like structure, displaying a central bulge with a smooth, diffuse halo. The core exhibits a concentrated luminosity, transitioning outwards into a less defined, fainter region. There is a noticeable ellipticity to the overall shape, with a ratio of approximately 8:1. Colors range from yellow-white in the center to redder hues within the halo, implying an aging stellar population and a potential reduction in active star formation. There's no visible spiral arm structure or dust lanes, suggesting a later stage of galaxy evolution. The galaxy does not show any signs of major interaction or merging activity and appears relatively undisturbed.
