The galaxy presents as a spiral galaxy, observed at a redshift suggesting a considerable distance. The spiral arms are prominent but somewhat diffuse, appearing flocculent in structure. The arms exhibit a blue hue, indicative of active star formation regions, likely containing young, massive stars. The galaxy's disk is oriented at an angle, offering a partial view of its structure. The central bulge is moderately sized and exhibits a yellowish tint, likely due to a higher concentration of older, less massive stars. There's no prominent bar structure visible. The galaxy appears relatively undisturbed, without major signs of ongoing merger activity, though there might be minor asymmetries suggesting past interactions or internal dynamics. The overall color profile suggests ongoing star formation, with a substantial population of older stars in the bulge.
