The galaxy appears to be a spiral galaxy, viewed at a slight angle. Definite spiral arm structures can be observed, although they are somewhat diffuse and not tightly wound. A bar-like structure is visible across the central region of the galaxy, oriented horizontally in the image. The bulge of the galaxy is relatively small compared to the overall size of the disk and is characterized by a more concentrated brightness. Patches of bluer light, suggestive of ongoing star formation, are observed within the spiral arms. There does not appear to be any significant morphological disturbance, indicating that the galaxy is relatively undisturbed.
