The galaxy presents a centrally concentrated, smooth morphology with an overall elliptical shape. The light distribution appears to be fairly uniform across the galactic body, exhibiting a predominantly yellow hue. There are no prominent spiral arms or dust lanes visible, suggesting a lack of significant ongoing star formation in well-defined disk structures. The galaxy's color index indicates a population of older stars, typical of elliptical galaxies at this redshift. The relatively smooth light profile suggests a system that has undergone significant merging in its history or has consumed most of its gas reservoir, leading to a cessation of star formation. There is a slight elongation of the galaxy, potentially indicating tidal interactions or a mild bar structure. The image analysis does not indicate any significant disturbances or ongoing major mergers.
