The galaxy exhibits a generally smooth, elliptical morphology. The central region is highly luminous and appears spheroidal. The luminosity decreases gradually from the core outwards, with no clear evidence of spiral arm structures or distinct features typically associated with disk galaxies. The overall color profile suggests an older stellar population, dominated by yellow and reddish hues, consistent with a low star formation rate. There are no obvious signs of active galactic nuclei or significant dust lanes obscuring the central region. The galaxy appears relatively undisturbed, with no major distortions or indications of ongoing mergers.
