The galaxy exhibits a clear spiral structure with prominent arms. These arms are well-defined and appear somewhat loosely wound. The disk is not perfectly face-on, showing a slight tilt, but it is not edge-on. There is some evidence of a bar-like structure crossing the galactic center, though it is not distinctly strong. The bulge component appears to be of moderate size, with a gradual transition into the disk. The color distribution suggests ongoing star formation within the spiral arms, which display a bluer hue compared to the more yellow-orange colored bulge. There may be minor disturbances present, possibly indicating past or ongoing interactions with neighboring galaxies.
