The galaxy presents as a centrally concentrated, elliptical-like structure, with a smooth light distribution and no apparent spiral arms or distinct morphological features. The core exhibits a significantly brighter luminosity than its surrounding halo, which gradually fades outward. The overall color appears to be slightly bluer in the central region, suggesting a younger stellar population or ongoing star formation, while the outer regions trend redder, potentially indicating older, redder stars. There is no obvious indication of active galactic nucleus activity, strong dust lanes, or tidal disturbances. The morphology appears largely undisturbed.
