This galaxy exhibits a disk morphology, viewed at an oblique angle, though not precisely edge-on. The spiral structure is readily apparent with well-defined arms. The central bulge is not dominant, appears small to moderate in size. Evidence of a bar structure is visible in the central region. The color profile suggests active star formation, indicated by bluer regions within the spiral arms. The overall form is relatively undisturbed, but hints of possible minor interactions are present. The galaxy does not appear to be undergoing a major merger.
