The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile. The central bulge appears yellowish-orange in color, indicating an older stellar population. Moving outward from the core, the galactic halo exhibits a gradual fading in luminosity. Some slight bluer light is visible in the outer regions, perhaps indicating the formation of more recent stars. There is no clear indication of spiral arms or a distinct disk. The overall shape appears moderately elliptical, rather than perfectly spherical or highly elongated. Close inspection reveals no obvious signs of major mergers or tidal disturbances, but there could be minor disturbances in the outer regions. The galaxy's moderate redshift indicates it is located at a significant cosmological distance. 
