The galaxy appears to be a spiral galaxy, seen at an oblique angle. It displays a central bulge that is moderate in size and possesses a yellowish hue, potentially indicating an older stellar population. The disk component is prominent, displaying defined spiral arms. The arms exhibit a relatively tight winding pattern and appear to be composed of a blueish color, suggesting active star formation within these regions. Evidence suggests the presence of two main spiral arms. There are no signs of a major merger event, but there are some minor disturbances.