The galaxy exhibits a clear spiral structure. Two prominent arms are visible, emanating from a bright central bulge. The winding of the spiral arms appears to be of medium tightness. The central bulge presents a moderate size relative to the disk. Evidence suggests the presence of a bar feature extending through the galactic center. The disk appears somewhat inclined to our line of sight, but not entirely edge-on. Overall the light appears to be composed of an intermediate to old stellar population, with some localized regions of recent star formation. There appear to be minor disturbances potentially caused by a recent minor merger or tidal interactions.
