The galaxy presents a prominent disk structure, viewed nearly face-on. Evident spiral arms emanate from the central region, exhibiting a moderately wound morphology. The color distribution suggests ongoing star formation within the spiral arms, indicated by a bluer hue. The central bulge appears relatively small and less prominent compared to the disk. There is no obvious bar structure visible. The galaxy displays no pronounced signs of tidal disturbances or interaction with other galaxies. Faint dust lanes are possibly present within the disk, obscuring some of the light. The overall light distribution suggests a morphology consistent with a late-type spiral galaxy, likely of type Sc.
