The galaxy exhibits a prominent disk structure, viewed nearly edge-on. A distinct dust lane is visible, bisecting the galaxy's luminous central region. The galaxy's color profile indicates a concentration of older stellar populations. The overall morphology suggests a system that has largely settled into a stable configuration, though with potential for continued star formation within the disk. There is no clear evidence of significant tidal interactions or ongoing mergers in the immediate vicinity. The general shape is fairly smooth, indicative of a generally elliptical form.
