The galaxy appears to be a spiral galaxy, observed at a moderate inclination. The central bulge is present, exhibiting a yellowish hue, suggesting an older stellar population. The disk is prominent and features well-defined spiral arms. These arms demonstrate a tight winding pattern. Traces of blue star formation regions can be observed within the spiral arms. The galaxy does not show any obvious signs of a major merger event, but the presence of minor disturbances within the disk cannot be ruled out. A bar structure is subtly suggested by the elongation of the central region, but it is not overwhelmingly prominent. The spiral arm count is difficult to precisely determine.
