The object presents as a spiral galaxy viewed at an oblique angle, showing a distinct disk structure. The spiral arms are readily apparent, exhibiting a loose, open winding pattern. Two dominant arms can be traced emanating from the central region. The central bulge appears relatively small compared to the disk, with a moderate level of brightness. There is evidence of a possible bar structure spanning across the central region of the galaxy. The overall color of the disk is bluish, suggestive of ongoing star formation. It appears as if there is an active star forming region within the center of this galaxy, shown by a brighter white center region. There may be a small amount of galactic disturbance, due to a non-uniform pattern in the spiral arms.
