This galaxy exhibits a moderately concentrated light profile, appearing largely smooth in structure. Its overall shape leans towards being somewhat rounded but with some intermediate features. There is little evidence of major mergers or significant disturbances in its morphology, although minor disturbances are possible. The color profile suggests a mix of stellar populations, with a dominance of older stars, giving it redder hues in some regions and bluer hues in others. Considering its redshift, it is a relatively luminous object with an estimated stellar mass that is substantial. The low star formation rate suggests it is evolving slowly, nearing the red sequence.
