The galaxy appears to be an early-type spiral galaxy, likely an Sa or Sb, seen at an oblique angle. A prominent bulge dominates the central region, displaying a smooth, orange-yellow color, indicating an older stellar population with little ongoing star formation. Fainter, bluer spiral arms are loosely wound around the bulge, but they are indistinct and less prominent than the bulge. The arms fade into the surrounding field, suggesting a low rate of star formation in the disk. Overall, the galaxy appears relatively undisturbed.
