The galaxy presents a largely smooth, elliptical morphology. The light distribution exhibits a centrally concentrated profile, with a gradual decrease in intensity moving outwards from the core. The dominant color appears to be a yellow-orange hue, indicating a population of older stars. There is a subtle hint of disk-like structure. No pronounced spiral arms or significant dust lanes are apparent. The galaxy is generally round in appearance, with little indication of tidal disturbances or ongoing merger activity. There is a faint blue region to the bottom corner of the galaxy which could indicate a small pocket of star formation. 