The galaxy presents a spiral morphology with a prominent central bulge. The spiral arms are well-defined, extending outwards from the bulge region. These arms are characterized by varying degrees of winding. Some arms appear tightly wound, while others exhibit a more open and loose structure. There is a clear disk that appears to be tilted relative to our line of sight. The galaxy exhibits variations in color. The central bulge has a yellow-white hue, whereas the outer regions of the disk show a blueish tint in the spiral arms. The blue color indicates the presence of younger, hotter stars. The galaxy displays some irregularities in its structure, possibly due to gravitational interactions or past mergers.
