The galaxy presents as a concentrated, centrally dominant structure, generally elliptical in shape. It exhibits a smooth texture with no apparent spiral arm structures or dust lanes discernible within the observed wavelengths. A slight elongation is apparent; it is neither perfectly spherical nor greatly elongated. The overall color appears subtly redder, with a yellowish hue emanating from the core region, suggesting a population of older stars. There is a complete lack of any signs of tidal disturbances, extended halos, or other indications of recent interactions with other galaxies. The morphological features suggest that the galaxy is most likely a relatively mature, quiescent system.
