The galaxy presents as a spiral galaxy with a notable disk component. It is observed at an inclined angle, but not fully edge-on. Two distinct spiral arms are discernible, appearing loosely wound and extending outwards from a central bulge. The bulge itself appears to be of moderate size, with a yellowish-white color. The arms contain a mixture of what appears to be newer star formation regions, indicated by a blueish-white color, and a more diffuse, yellowish-red component. A possible central bar structure is suspected due to the elongated shape near the core. The overall structure suggests a galaxy that is not currently undergoing a major merger, though minor disturbances cannot be ruled out based on visual inspection alone. The surface brightness profile transitions smoothly from the bulge to the disk.
