The galaxy presents as a relatively smooth, elliptical morphology. The central bulge exhibits a concentrated, yellowish-white hue, suggesting a population of older, cooler stars. Moving outward from the core, the color gradient shifts towards a more greenish tinge, possibly indicating the presence of some younger stars or ionized gas, although the overall star formation rate appears to be low. There is no clear evidence of spiral arms or significant dust lanes. The shape is generally rounded, with a slight deviation from perfect circularity. No major merger events or significant tidal disturbances are apparent, although some minor asymmetries or disturbances cannot be entirely ruled out based on the image resolution. The galaxy extends across a moderate angular size in the image, suggesting a considerable physical size given its estimated redshift.
