This galaxy exhibits a clear spiral structure, characterized by two well-defined spiral arms emanating from a central bulge. The spiral arms display a moderately wound morphology. The central bulge appears to be of moderate size relative to the overall galactic disk. There is no obvious visual sign of a strong bar structure, but the possibility of a weak bar cannot be entirely ruled out. The galactic disk appears somewhat perturbed, with the possibility of minor disturbances, though no clear indication of a major merger is evident. The color distribution suggests active star formation within the spiral arms, as indicated by the presence of blue regions. The overall structure indicates this is likely a relatively normal spiral galaxy at intermediate redshift.
