The galaxy appears as a moderately elongated, disk-shaped structure. Its morphology suggests a spiral galaxy, though the spiral arms are not clearly defined in this image. The central bulge is not highly prominent, appearing relatively small and indistinct. The overall color profile indicates a mixture of stellar populations, with a slightly bluer hue in the disk and a yellower tint near the center. This color variation could suggest ongoing star formation in the disk, with older, redder stars concentrated in the bulge. There are no obvious signs of major disturbances or mergers affecting the galaxy's morphology.
