The galaxy presents a spiral morphology with a prominent central bulge. The spiral arms appear loosely wound and are somewhat patchy in appearance. The overall color suggests active star formation within the disk, although the bulge appears yellower, indicating an older stellar population. There's a subtle suggestion of a bar structure crossing the center of the galaxy, with two main arms emanating from near the ends of the bar. No major signs of tidal disturbance or ongoing merger activity are immediately apparent, although there might be minor irregularities in the arm structure indicating slight gravitational interaction. The disk is viewed at an angle, not quite edge on, allowing for the spiral arms to be seen clearly. The central bulge appears to be of moderate size compared to the overall disk of the galaxy.
