The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge with a notable decrease in luminosity towards the outer regions. The color profile suggests a relatively evolved stellar population, with a yellowish-orange hue dominating the core, transitioning to slightly redder tones in the periphery. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy appears undisturbed, lacking any indications of ongoing major merger activity or tidal distortions. A high degree of central sphericity is observed with no apparent elongation or asymmetries, this indicates that the galaxy is likely a relaxed system. Overall, this galaxy appears as a typical elliptical galaxy at a considerable cosmological distance.
