This galaxy exhibits a distinct spiral structure. Two well-defined spiral arms emanate from a bright, moderately sized central bulge. The arms appear loosely wound, extending outwards from the core with a somewhat flocculent appearance. The color of the central bulge appears more yellow-white, suggesting an older stellar population. Conversely, the spiral arms exhibit a bluer hue, indicative of ongoing star formation. The galaxy's disk is not perfectly face-on, presenting a slightly tilted view from our vantage point. There is no indication of significant merger activity or tidal disturbances. The image suggests a well-formed spiral galaxy undergoing active star formation within its arms.
