The galaxy presents as a generally elliptical structure, elongated along its major axis. A concentrated central bulge region exhibits a yellowish-white hue, suggesting an older stellar population dominating the core. Moving outward from the center, a subtle color gradient is observed. The outer regions appear bluer, hinting at the presence of younger, hotter stars or ongoing star formation. The overall smoothness of the light distribution suggests a relatively evolved system with a potentially quenched or slowly declining star formation rate. There is very little morphological indication of spiral arms or significant dust lanes, further supporting the notion of an evolved galaxy morphology. Minor disturbances cannot be ruled out, but the structure appears primarily relaxed with no major mergers visibly apparent. The galaxy size is intermediate for this redshift.
