The galaxy presents a disk-like morphology, viewed at an angle that is not quite edge-on. Spiral arm structure is visible, appearing somewhat patchy and not tightly wound. There seems to be a dominant bulge component, moderately sized and centrally located. The disk component has a distinct, though not highly disturbed, structure. The light distribution appears bluer in some regions of the spiral arms. There might be ongoing, minor interaction or disturbance but the morphology is not indicative of a major merger event. No strong bar feature is apparent in the central region.
