This galaxy appears to be a spiral galaxy, presenting with prominent, well-defined spiral arms. The arms exhibit a notable degree of symmetry, appearing to wind moderately tightly around the central bulge. The bulge itself is a significant feature, though not overwhelmingly dominant, and it is noticeably bright and concentrated. There may be a bar-like structure contributing to the galaxy's morphology, although its presence is not definitively confirmed. The disk is not edge-on, offering a face-on view of the spiral structure. The color distribution suggests active star formation regions distributed throughout the spiral arms, particularly in blue wavelengths, with a noticeable reddish component concentrated toward the central bulge, indicative of an older stellar population. The overall structure does not show signs of significant recent merger events, although minor disturbances cannot be ruled out.
