The galaxy presents as a disk galaxy seen nearly edge-on. There's a prominent dust lane bisecting the galaxy, obscuring light from the galactic center. The bulge appears extended and predominantly rounded. There are no obvious signs of recent major mergers or strong tidal disturbances present in the image, though some minor distortions are possible. The color suggests a mix of stellar populations, with bluer regions possibly indicating ongoing star formation and redder regions possibly indicating older stellar populations. Overall, the galaxy exhibits features consistent with a relatively undisturbed, late-type spiral galaxy observed at a significant distance.