This galaxy presents an edge-on disk morphology. The dust lane is prominent, bisecting the galaxy along its major axis and obscuring the central region. The bulge appears relatively small and somewhat boxy. It exhibits a redder color index than the surrounding disk, which is more blue, suggesting an older stellar population. The disk extends a significant distance from the bulge, and the overall appearance is relatively undisturbed, showing no signs of recent major mergers, although there may be some minor disturbance or tidal features present at the limits of the disk. The overall luminosity suggests a substantial stellar mass, with ongoing, but not particularly intense, star formation activity.