The galaxy presents as an edge-on spiral, exhibiting a prominent and extended disk. The central bulge appears significantly brighter and more concentrated than the rest of the disk, with a rounded morphology. Dust lane is apparent along the major axis of the disk, obscuring light and dividing the galaxy into upper and lower halves. The color profile shows bluer hues at the edges of the disk, indicating recent star formation. The redder color of the bulge suggests an older stellar population. There is no distinct evidence of major merger activity or strong tidal distortions in the disk.
