The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its color gradient appears to transition from a bluish-white core to a more yellowish-red outer halo. There are no readily discernible spiral arms or distinct features suggestive of active star formation regions. The galaxy's overall structure is somewhat elongated, deviating slightly from perfect sphericity. There are no apparent signs of tidal disturbances or major interactions with nearby galaxies. Faint asymmetry could indicate a minor merger, or simply be related to internal dust extinction. The light profile suggests an older stellar population dominating the central regions with a gradual transition to perhaps a younger or dustier stellar population in the outskirts. The object exhibits a redshift indicative of a considerable distance, suggesting an evolved system with a moderate stellar mass.