The galaxy presents a somewhat edge-on disk morphology. A central bulge region is visible with a yellowish-orange hue, suggesting a population of older stars. The disk exhibits a bluer coloration extending outwards from the bulge, indicative of ongoing star formation. There are hints of dust lanes within the disk, although the image resolution limits detailed observation. The galaxy appears relatively undisturbed, without any obvious signs of major mergers or tidal interactions. Overall, the galaxy appears to be a spiral galaxy, possibly undergoing moderate star formation.
