The galaxy presents as an edge-on disk galaxy. There is a prominent central bulge that appears to be somewhat rounded. Evidence of a disk is clearly visible, with the galaxy elongated along a single axis. The light distribution suggests significant obscuration, likely due to dust lanes within the plane of the disk. The color distribution indicates a mix of stellar populations, with a redder bulge and bluer outer disk regions. Based on its redshift, this galaxy is relatively distant. There is no obvious indication of a major merger event; however, minor disturbances cannot be ruled out. The overall morphology suggests a relatively evolved system.
