This galaxy appears to be a disk galaxy viewed edge-on. The dust lane is prominent, obscuring the central bulge. The bulge appears to be rounded. There may be a slight warp present in the disk. The overall color is indicative of a population with slightly older stars. There are areas that suggest regions of active star formation as well. There appears to be a larger galactic body with a smaller one interacting with it, which suggests it may be a galactic merger event.
