The galaxy exhibits a distinct spiral structure, with two prominent arms emanating from a central bulge. The spiral arms appear loosely wound and extend significantly outwards from the bulge, showing a patchy distribution of star formation regions. The bulge itself is of moderate size, contributing visibly to the overall luminosity of the galaxy. A bar structure is present across the galaxy, but appears weak. There is a possible minor disturbance in the overall morphology suggesting recent or ongoing interaction with another galaxy. The overall color index suggests active star formation within the disk.
