The galaxy presents as a spiral type, exhibiting a distinct disk structure. The arms are well-defined, with a moderate winding pattern, appearing neither tightly wound nor particularly loose. The color suggests active star formation, particularly noticeable in the spiral arms. The central bulge is moderately sized, with a less prominent presence than the arms. The galaxy does not appear to be strongly barred. There are hints of minor disturbances in the galactic disc, but the overall form is largely undisturbed. 
