The galaxy presents as a spiral type, viewed at an angle slightly inclined from face-on. Two prominent spiral arms are clearly discernible, with a moderate winding, displaying both medium tightness. A bar structure is present, appearing relatively strong. The central bulge component seems comparatively small to moderate in size, with some concentrated luminosity. The overall disk structure appears dominant, with a relatively smooth texture to the disk. Evidence of minor tidal disturbance or interaction may be present in the form of faint, asymmetric light distribution in the outer regions.
