The galaxy presents as an edge-on spiral, exhibiting a clearly defined dust lane bisecting the central bulge. The bulge appears somewhat elongated and displays a smooth texture, suggesting a relatively older stellar population concentrated towards the center. 

The galactic disk appears thin and extended, displaying blue hues indicative of ongoing star formation. The overall structure suggests a moderate inclination relative to the observer's line of sight. There may be subtle, minor disturbances visible within the disk, but these are not obviously indicative of an ongoing major merger event. The bulge shape appears somewhat rounded, though a hint of boxiness cannot be completely ruled out.
