The galaxy appears to be a spiral galaxy observed at an angle. It is elongated, with the major axis significantly larger than the minor axis, suggesting a highly inclined disk. There appears to be a central bulge, slightly brighter and more concentrated than the rest of the disk. The arms are not well-defined but show hint of star formation activity. The spiral structure is not grand design, and the galaxy appears to be fairly compact. The colours suggest relatively old stellar populations dominating the galaxy. The morphology suggests it is unlikely to be undergoing a major merger or to show significant tidal disturbances. The light emitted by this object is redshifted.
