The galaxy presents a disk-like structure, viewed at an angle slightly inclined from face-on. Prominent spiral arms emanate from the central region. The winding of these arms appears to be tightly wound. The bulge component appears relatively small compared to the overall disk size. The galaxy exhibits a blue hue in the outer regions of the disk, suggesting ongoing star formation. The central region displays a yellower, more concentrated light distribution, indicative of an older stellar population and a possible galactic bar structure, though subtle. There is no clear indication of any major ongoing merger events, though a minor tidal disturbance cannot be ruled out. Overall, it appears to be a late-type spiral galaxy with a relatively low Sersic index, indicating a disk-dominated morphology. The overall ellipticity of the galaxy is not far from circular.
