The galaxy presents a distinct spiral structure. Two prominent spiral arms are clearly visible, exhibiting a loose winding pattern. The galaxy's disk is oriented at an angle that is not quite edge-on, but not fully face on either, allowing for observation of its spiral morphology. The central bulge appears relatively small to moderate in size, with a yellow/orange hue suggesting an older stellar population. Blue and green tinges are present throughout the disk and spiral arms, indicative of active star formation regions. Overall the galaxy shows signs of disturbance or potential merging activity, with an irregular shape that's slightly hard to focus. The light emitted is red-shifted suggesting it is far away. 
