The galaxy presents as a spiral galaxy with a relatively bright, concentrated central bulge. Spiral arms are clearly visible extending outward from the central region, displaying a moderate degree of winding. The arm structure indicates the presence of at least three discernible arms. The bluer coloration observed within the spiral arms suggests ongoing star formation activity. The galaxy does not appear to be strongly barred, if barred at all. It has a small-to-moderate sized bulge relative to the disk. Overall, the morphology appears largely undisturbed, with no readily apparent signs of a major merger event.
