The galaxy presents as a relatively face-on spiral galaxy at a moderate redshift. It exhibits a distinct, albeit somewhat diffuse, spiral arm structure with at least two prominent arms emanating from a central bulge. The arms appear loosely wound and feature a mix of blue and reddish-orange hues, indicative of both ongoing star formation and older stellar populations. The central bulge is prominent with a yellowish color suggesting a concentration of older, redder stars. The overall color profile suggests a significant population of younger stars in the spiral arms. There is no apparent strong bar structure visible. Slight asymmetry is visible, possibly indicating gravitational interactions or ongoing mergers.
