This galaxy exhibits a spiral morphology, characterized by a central bulge and a prominent disk. The bulge appears yellowish-orange in color, suggesting an older stellar population, while the disk displays a bluer hue, indicative of ongoing star formation. Two well-defined spiral arms emerge from the central bulge, wrapping around the galaxy in a relatively tight configuration. These arms show clumpy structures with star forming regions and dust lanes. There is no strong evidence of a bar structure bisecting the bulge. There are a few minor disturbances in its form, but it does not appear to be undergoing a major merger. Overall, the galaxy presents a well-defined spiral structure with clear indications of active star formation within its arms.
