The galaxy presents as a face-on spiral galaxy, exhibiting a dominant central bulge that graduates smoothly into what appears to be a prominent disk. The bulge displays a yellow-orange hue, suggestive of an older stellar population and lower rates of current star formation.

The disk component shows hints of spiral arm structure, although these are not sharply defined. There is a mottled appearance in the disk, possibly indicating regions of star formation, although this is not as pronounced as in some other spiral galaxies. The overall color of the disk appears more blue/green than that of the central bulge, indicative of the presence of younger, hotter stars. Overall, this galaxy appears to be a fairly large, disk-dominated spiral at intermediate redshift.