The galaxy appears to be a spiral galaxy, exhibiting a pronounced disk structure with clearly defined spiral arms. Two main arms are visible, tracing a relatively open winding pattern. The central bulge presents a moderate size compared to the disk. Indications of a bar structure are present, though somewhat subtle. The disk displays variations in color and luminosity, suggesting regions of active star formation interspersed with older stellar populations. There is a possible companion galaxy or dwarf galaxy to the right, but it is not certain if it's interacting. No signs of major disturbances or ongoing mergers are immediately apparent. The galaxy is viewed at an angle, not edge-on. 
