The galaxy appears as a single, relatively smooth concentration of light. It exhibits a generally elliptical morphology, appearing mostly round in shape. There is no apparent disk structure or spiral arms. The galaxy's color profile suggests a relatively evolved stellar population, with a yellowish-orange hue indicative of older stars dominating the light output. There are no prominent features suggesting ongoing major mergers or tidal disturbances, although minor disturbances can not be ruled out based on the image. Given the redshift, the physical size of this galaxy appears to be of considerable scale. The observed smoothness further indicates a relatively quiescent system with a low rate of star formation.
