The galaxy in question exhibits a clear spiral structure. The spiral arms appear well-defined and moderately wound. Two prominent spiral arms seem to dominate the structure. The central bulge is of moderate size, with a yellow color indicating an older stellar population. The disk component shows blue areas, possibly indicating ongoing star formation. There is no evidence of a strong central bar. The galaxy appears relatively undisturbed, exhibiting no major signs of mergers, although some minor disturbances cannot be ruled out. The galaxy shows a relatively high inclination.
