The galaxy appears to be a spiral galaxy, observed at a slight inclination. It exhibits a central bulge that is yellowish-white, with a moderate size. The arms are fairly tightly wound and are light blue in color, indicating the presence of younger, hotter stars and ongoing star formation. There is no apparent bar structure, and the galaxy shows no signs of a major ongoing merger, although some minor disturbances may be present. Overall, the galaxy appears to be in a relatively quiescent state of evolution.
