The galaxy appears as a disk galaxy, observed nearly edge-on. The disk exhibits a relatively smooth texture. A central bulge is prominent, appearing somewhat rounded. There is no apparent evidence of a bar structure. The morphology indicates this galaxy has likely undergone no recent major mergers, but there is a slight chance it has undergone some minor disturbance. This is likely a relatively massive galaxy that has little to no current star formation. The galaxy is most luminous in the redder wavelengths. 
