This galaxy presents a complex morphology characterized by both smooth and structured features. The central region exhibits a high degree of luminosity, suggestive of an older stellar population or potential AGN activity. There is evidence of spiral arm structures, albeit somewhat disrupted. These spiral arms display a patchy distribution of star formation regions, which appear in the image as areas with bluer hues, particularly on the northern side. The disk is likely inclined relative to our line of sight, but it is not an edge-on galaxy. Furthermore, the galaxy exhibits signs of gravitational interaction, such as tidal tails and possible disturbance of the disk, indicating either an ongoing or recent merger event with a companion galaxy. Overall, the galaxy presents a dynamic and possibly evolving system.