The galaxy appears to be a spiral type, exhibiting a disk-like structure with observable spiral arms emanating from a central bulge. The spiral arms are somewhat flocculent, and there appears to be some degree of disturbance in the overall morphology, possibly indicating an interaction or merger event. The central bulge has a moderate size relative to the disk and displays a yellowish hue, suggesting an older stellar population. The disk shows bluer regions indicative of ongoing star formation, particularly along the spiral arms. The galaxy is not perfectly face-on; it's inclined relative to our line of sight. Overall the galaxy appears to be experiencing active star formation and may be undergoing gravitational interaction with another galaxy or experiencing a post-merger phase.
