The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a concentrated, bright yellow-white core, likely indicating an older stellar population and minimal ongoing star formation. The outer regions appear less luminous, with a gradual decrease in intensity moving outwards from the core. The overall shape is predominantly round, with only a slight deviation from perfect circularity. There is no apparent evidence of spiral arms, bars, or significant dust lanes. No major mergers or tidal disturbances are visually discernible, although subtle asymmetries in the outer halo cannot be ruled out without further analysis. The color profile suggests a red-sequence galaxy dominated by evolved stars. The apparent size is small, indicative of a distant object, consistent with its redshift.
