The galaxy presents a spiral morphology, although the relatively low resolution of the image makes it difficult to discern fine details. There is a prominent central bulge which appears yellowish, potentially indicating an older stellar population. Emanating from the bulge are two distinct spiral arms. These arms display a moderate pitch angle, neither tightly wound nor particularly loose. Some segments of the spiral arms appear clumpy, suggestive of active star formation regions. There are two primary arms that appear to begin at each end of the bulge, which are relatively uniform in color. There is no strong evidence of a bar structure within the galaxy. Overall, the galaxy appears relatively undisturbed, without obvious signs of a recent major merger event, though minor irregularities cannot be ruled out based on this single image. The color gradient suggests a range of stellar populations, with the bulge dominated by older, redder stars and the arms potentially containing younger, bluer stars.
