The galaxy presents as a spiral galaxy with a discernible disk structure, exhibiting active star formation regions. Two well-defined spiral arms are visible, displaying a moderate winding pattern. The central bulge is moderately sized, with a subtle bar-like feature running through it. Evidence of ongoing or recent minor disturbance can be seen in the outer regions of the disk, though the primary structure appears relatively unperturbed. The disk is observed face-on, allowing for clear observation of its features. The presence of HII regions suggests recent or current star formation, but at a relatively low rate. Overall, the galaxy appears as a normal spiral galaxy at intermediate redshift, with a moderate stellar mass.