The galaxy appears as a centrally concentrated, luminous object. Its overall form is predominantly smooth, with little discernible internal structure or spiral arm features visible in this image. The light profile appears largely elliptical and fairly rounded, indicating a minimal degree of elongation. A slight color gradient is observed, with a bluer hue in the central region, transitioning to redder tones towards the outer edges. This could suggest ongoing star formation in the core, or a difference in stellar populations, with younger, hotter stars concentrated towards the center. There are no indications of major disturbances or tidal features suggesting a recent major merger. The overall appearance suggests a relatively relaxed morphology for a galaxy at its estimated redshift.
