The galaxy appears to be a spiral galaxy, exhibiting a distinct disk structure. Spiral arms are visible, tightly wound around a central bulge. The bulge appears moderately sized. The disk appears to be viewed nearly face-on. The color gradients within the galaxy suggest ongoing star formation, particularly within the spiral arms. The overall color of the galaxy appears bluer in the spiral arms and the nuclear region appears to be more red. There does not appear to be a strong central bar feature. The galaxy does not show obvious signs of recent major merging activity, however there may be minor disturbances in the disk structure that could be due to a smaller gravitational interaction.
