The galaxy exhibits a clear disk structure with prominent spiral arms. These arms display a distinct winding pattern, appearing moderately wound. There appears to be two main spiral arms emanating from the central region. There is evidence of a stellar bar structure spanning the central region of the disk. A small bulge is present but does not dominate the overall galactic structure. No signs of major mergers are apparent, although some minor disturbances within the disk cannot be ruled out. The galaxy appears to be relatively undisturbed, with a well-defined structure.
