The galaxy presents a disk-like morphology with evidence of spiral arm structure. The arms appear somewhat flocculent and are of a blueish tinge, suggesting ongoing star formation. There is a prominent central bulge that presents a yellow-orange color, indicative of an older stellar population and/or dust obscuration. The bulge appears to be moderate in size relative to the disk. The galaxy is observed at an angle away from edge-on, but has no clear signs of strong tidal disturbances or major merger activity. A hint of a bar may be present, but it is not the dominant feature.
