The galaxy appears to be a spiral galaxy viewed at an oblique angle. It exhibits a flattened, disk-like structure. There is a central bulge that appears relatively smooth and concentrated.

Evidence of spiral arms can be seen, with some asymmetry in their distribution. The arms have a clumpy or patchy appearance. Some regions have bluer hues, potentially indicating areas of active star formation. The overall color gradient suggests the presence of a mixed stellar population with varying ages. There may be some disturbance and signs of tidal interactions.
