The galaxy presents as a spiral type, although the inclination obscures a clear view of the disk structure. A central bulge is visible, possessing a moderate size relative to the overall galactic structure. The spiral arms are prominent and defined by a blue hue, possibly indicating regions of active star formation. The winding of the spiral arms appears relatively tight. Evidence suggests the presence of a bar structure across the bulge. The galaxy exhibits a slight disturbance in its morphology, hinting at a possible minor interaction or recent merger event.
