The galaxy presents a somewhat face-on spiral morphology. The central bulge is visible, though not overwhelmingly prominent, indicating a possible intermediate bulge size. Spiral arms are discernible, exhibiting a relatively open structure and moderate winding. The disk of the galaxy appears relatively smooth and featureless, with a hint of some star forming regions within the arms. There appears to be a lack of substantial dust lanes or prominent knots of star formation. The galaxy exhibits no obvious signs of a recent major merger event, or significant tidal disturbances in its overall structure. The colour of the galaxy suggests a intermediate redshift, which is also verified by the data.
