The galaxy presents as an edge-on spiral with an apparent redshift. It displays a prominent central bulge region that appears rounded. There is evidence of a disk structure, oriented nearly edge-on. The outer regions of the disk appear somewhat fainter and less defined.  The system shows no obvious signs of major mergers, but there may be some minor disturbances visible. There seems to be a low level of star formation activity within the disk. The light distribution suggests a significant stellar mass.