The galaxy appears to be a spiral galaxy, viewed at an oblique angle. There is a noticeable bulge at the center with a more diffuse spiral structure emanating from it. The spiral arms show signs of ongoing star formation regions as indicated by the blueish hue and the slight irregularities. Although difficult to tell with this resolution, there is a chance of minor galactic interactions but nothing that indicates a full merger. The color profile indicates average light for a galaxy at this redshift.
