The galaxy appears to be a spiral galaxy with a prominent central bulge. While the bulge is apparent, it does not dominate the overall structure, suggesting it might be moderate in size. Spiral arms are clearly visible and relatively tightly wound. The disk is oriented somewhere between face-on and slightly inclined. There may be some slight disturbances in the arms, which could be evidence of minor gravitational interactions with another galaxy, but no obvious signs of major mergers or severe disturbances are seen. There does not appear to be a strong central bar structure. The color suggests a mix of stellar populations, including both older, redder stars in the bulge and younger, bluer stars in the spiral arms. Overall, the galaxy presents a typical spiral morphology.