The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology, although subtle deviations suggest a possible disk-like structure viewed at a shallow inclination. The central region exhibits a bright, yellowish-white core, likely indicating an older stellar population concentrated in the bulge. The overall color profile suggests a moderate redshift, with an apparent suppression of bluer wavelengths. Faint extensions surround the core, and subtle spiral arm hints are present within them. These extensions also demonstrate a slightly bluer hue than the central bulge, potentially indicating the presence of younger stars or ongoing star formation. There is no apparent evidence of major ongoing mergers or significant tidal disturbances, but there are minor asymmetries that could be indicative of a past interaction.
