The galaxy presents as a spiral type, exhibiting a disk-like structure with distinct spiral arms. These arms appear loosely wound, extending outward from the galactic center. Within these spiral arms, there is evidence of star formation regions, indicated by localized areas of bluer light, possibly associated with younger, hotter stellar populations. A faint bar structure seems present across the central bulge. The central bulge itself seems to be of moderate size, and it contributes significant brightness to the galaxy. There is no clear indication of a recent or ongoing major merger event.