The galaxy presents as a largely featureless, smooth elliptical galaxy, likely at a significant distance. Its overall morphology appears spheroidal, exhibiting high ellipticity. The galaxy has a distinct color gradient, shifting from a yellow-white hue at its core to a faint blue in the outer regions. This transition is indicative of a central concentration of older stellar populations, with the bluer peripheral regions suggesting ongoing, albeit subdued, star formation. The galaxy is well-defined, exhibiting no discernible tidal disturbances or merging signatures. No distinct spiral arms, bars, or other detailed structures are visible. The light distribution is centralized and gradually diminishes with distance from the nucleus.