The galaxy presents as a spiral galaxy viewed at an oblique angle, appearing nearly face-on. Evident spiral arm structure extends from a moderately sized central bulge. The arms exhibit a patchy distribution of star-forming regions, indicated by variations in luminosity and subtle color differences across the disk, suggesting on-going star formation. There is a slight hint of a bar structure in the central region, although it does not appear to be particularly pronounced. The galaxy is relatively isolated, showing no signs of major interaction or merging events. The light distribution is dominated by a somewhat diffuse component, hinting at an extended stellar disk.
