The object appears to be a spiral galaxy, presenting a disk-like structure with a noticeable central bulge. The spiral arms are prominent, with some exhibiting a tightly wound morphology, while others appear more open and loosely defined. Overall, it seems to have two main spiral arms, but some appear less distinct. The central bulge appears yellowish-orange, suggesting an older stellar population. The disk shows a bluer hue, indicating the presence of younger stars and ongoing star formation within the spiral arms. There are some apparent disturbances, though they do not indicate a major merging event. A bar is present, however its difficult to determine if its a strong or weak bar based on this image. The galaxy presents a moderate inclination with respect to our line of sight. The galaxy exhibits a relatively small bulge.
