The galaxy appears to be a spiral galaxy, seen at an intermediate angle. There is evidence of a central bulge, which appears yellowish in color, suggesting an older stellar population. The disk shows some distinct spiral arm structure. The spiral arms appear bluish, indicating the presence of younger, hotter stars and star formation regions. There appears to be a slight asymmetry to the disk, which may indicate a minor interaction or disturbance. The galaxy is neither perfectly smooth nor extremely disturbed; it shows features of a spiral disk with some irregularities.
