The galaxy exhibits a clear disk morphology, viewed at an oblique angle, but not quite edge-on. There appears to be evidence of spiral arms. The disk component dominates the galaxy's visual structure. There is no strong bar feature visible in the central region. The bulge appears small to moderate in size. The overall color suggests ongoing star formation, with some bluer regions apparent. There is also evidence for a minor merging event, which appears to be causing disturbances in the primary body.
