The galaxy presents a clear spiral morphology. Two distinct, prominent spiral arms extend outwards from a bright, moderately sized central bulge. The winding of the spiral arms appears to be relatively loose, with a significant portion displaying a medium winding. The colour distribution suggests some active star formation within the spiral arms, though possibly not intensely so. The galaxy appears generally undisturbed, without significant signs of recent major merger activity, although a very minor asymmetry or irregularity may be present. The disk is face-on, so we are presented with the galaxy's full morphological features. Bar structure seems subtle, perhaps a weak bar feature.
