The galaxy appears to be a spiral galaxy, viewed at a moderate inclination, not quite face-on nor edge-on. Evident spiral arm structure is present, though somewhat flocculent and not tightly wound. The central bulge region is prominent with a moderate size relative to the disk, exhibiting a yellowish hue indicative of an older stellar population. A subtle bar may be present, but it's not a dominant feature. The disk shows a bluer color, consistent with more recent star formation. There are no obvious signs of a major merger event, though some minor disturbances cannot be ruled out based on this image.
