This galaxy exhibits a smooth, elliptical morphology. The central bulge appears prominent and intensely luminous, displaying a yellowish-orange hue, likely indicative of an older stellar population. Fainter, extended regions surround the core, creating a halo-like structure. The overall shape is moderately elongated, with the major axis extending horizontally. The galaxy appears relatively undisturbed, showing no signs of recent major mergers or significant tidal interactions. There is a subtle colour gradient, with the outer regions displaying hints of bluer light, suggesting the presence of some younger stars, however they are quite faint. The galaxy is a considerable distance away, inferred from its small angular size despite its high luminosity, and a likely high stellar mass. The rate of star formation is probably low.