The observed galaxy presents as an edge-on spiral, likely at a redshift around 0.14. The pronounced dust lane bisecting the galactic plane indicates significant obscuration and confirms the presence of a substantial disk component. A central bulge is apparent. It appears relatively prominent and rounded. The overall colour gradient shifts from a more yellow-orange hue in the central bulge region to a bluer colouration further out in the disk, suggesting on-going or recent star formation within the disk. There are no prominent signs of recent or on-going major mergers, but potentially a minor irregularity.
