The galaxy presents as a spiral galaxy, observed at a slight inclination from an almost face-on orientation. The galaxy exhibits a prominent central bulge. The spiral arms appear somewhat flocculent, displaying a patchy structure with regions of increased luminosity which may indicate active star formation. Overall, the galaxy appears to be relatively undisturbed with no apparent signs of a major merger, although some minor disturbances are possible. A weak bar feature is suspected to be present in the central region. The dominant colors observed in the disk are indicative of ongoing star formation, exhibiting bluer hues, while the central bulge appears more yellow.
