The galaxy exhibits a clear spiral structure. The spiral arms appear somewhat tightly wound, exhibiting a largely flocculent structure. There appears to be at least three discernible spiral arms. The central bulge exhibits a moderate size. A weak bar structure appears present within the bulge. The disk is viewed approximately face-on. No major signs of ongoing mergers or strong tidal disturbance are readily apparent, though subtle irregularities may suggest minor gravitational interactions. The galaxy's color indices suggest moderate star formation activity. The overall morphology suggests a late-type spiral galaxy.
