This galaxy presents a distinct spiral structure. The spiral arms are well-defined and appear loosely wound, extending outward from a central region. A noticeable asymmetry is present, potentially indicating an ongoing interaction or past merger event. The blue hue within the arms suggests the presence of active star formation regions with young, hot stars. The galaxy exhibits a slight bulge at the center, though it does not dominate the overall structure. Evidence of a bar feature is not immediately obvious. There are visual hints of disturbances in the morphology, such as extended or irregular features. The overall color profile indicates a mixture of stellar populations, from the younger, bluer stars in the arms to potentially older, redder stars in the bulge and inner regions.
