The galaxy presents as a spiral galaxy with a moderately inclined disk. There's a central bulge region that appears relatively smooth and concentrated. The spiral arms are not sharply defined but appear somewhat flocculent, displaying patchy star formation regions with what appear to be some HII regions present, indicated by the greenish hue concentrated in the lower section of the galactic disk. These active regions seem to suggest ongoing star formation. The overall color gradient transitions from the redder central bulge to bluer outer arms. The structure appears to be mostly undisturbed with a reasonable level of symmetry.
