This galaxy presents a somewhat flocculent spiral structure. The spiral arms are not sharply defined but appear patchy and less continuous. The arms show a blue tint, suggesting active star formation regions. There's a central bulge of moderate size. The overall disk of the galaxy is not precisely edge-on, and no strong bar structure is observed. There is some indication of potential interaction or a minor disturbance, but the morphology does not overwhelmingly suggest a major ongoing merger.
