The galaxy presents as a single, centrally concentrated object, with a generally smooth profile. There is a distinct color gradient present, trending from yellow-orange towards the center, to a greenish-white hue in the outer regions. The galaxy is largely elliptical in shape, displaying a very high degree of roundness. There is no evidence of spiral arm structures or a prominent disk. The galaxy appears undisturbed, with no obvious signs of recent or ongoing mergers or tidal interactions. The galaxy possesses an estimated mass of approximately 10^10.7 solar masses and has a low star formation rate.
