The galaxy in the image appears to be a spiral galaxy, viewed at an oblique angle, possibly with a slight edge-on presentation. There is a central bulge that shows a yellow-white coloration, suggesting an older stellar population with lower ongoing star formation. Fainter spiral arms extend from the central bulge, showing some blue coloration that implies the presence of younger stars. A slight warping may be present in the disk. There is some clumpy structure along the arms, potentially indicating areas of active star formation. The overall morphology suggests a fairly well-defined disk, despite some signs of possible disturbance.
