The galaxy presents as an edge-on spiral, with a prominent and elongated disk. The central bulge appears bright and somewhat rounded, possibly indicating a significant population of older stars. The disk displays a color gradient, appearing reddish-orange towards the center and gradually transitioning to bluish hues at the outer edges. This suggests ongoing star formation in the outer regions, contrasting with a possibly older stellar population concentrated in the core. There are no immediately obvious signs of major mergers or significant tidal disturbances, though subtle irregularities within the disk cannot be ruled out with the available image resolution. The galaxy shows a moderate amount of star formation.
