The galaxy presents as a highly inclined, edge-on spiral. The central bulge appears prominent and concentrated, exhibiting a smooth, rounded morphology. The disk is observed to be thin and elongated, characteristic of edge-on spiral galaxies. There is a suggestion of a dust lane bisecting the galaxy along the plane of the disk, although resolution limitations prevent definitive confirmation. The overall color profile suggests a population of older stars, particularly within the central bulge. Faint hints of bluer hues near the outer edges of the disk may be indicative of ongoing, albeit modest, star formation activity in these regions. No significant signs of major disturbances or ongoing mergers are apparent in this image, however, there may be some disturbances.
