The galaxy appears to be a spiral galaxy, viewed at an angle that is neither face-on nor edge-on. The central bulge is prominent and moderately sized, exhibiting a bright, concentrated glow. The spiral arms are somewhat diffuse and not sharply defined, but visible extending from the central region. There is a suggestion of spiral structure present, although it is not overwhelmingly distinct. The disk component dominates the overall appearance, with a smoother appearance than typical spirals. No clear bar structure is present. There appears to be no sign of strong galactic merging. There may be a minor disturbance in the morphology, but the galaxy is generally well-formed.
