The galaxy presents a distinct disk morphology, viewed at an oblique angle relative to our line of sight. A central bulge is visible, appearing moderately prominent and ellipsoidal. Spiral arm structures are discernible within the disk. These arms exhibit a multi-armed pattern, with a majority displaying two prominent arms. The winding of these arms appears to be tightly wound toward the center. A weak bar-like structure might be present within the central region, intersecting with the bulge. Overall, the galactic structure appears relatively undisturbed with no major signs of mergers or interactions. The dust lanes and star formation regions are also visible throughout.
