This galaxy exhibits a morphology consistent with a spiral type. The object presents a discernible disk, viewed at an angle slightly offset from edge-on. There is evidence of spiral arm structure within the disk component, with the arms appearing somewhat loosely wound. A central bulge is present, though it appears relatively small and not overwhelmingly dominant in size compared to the disk. The overall color suggests a mix of stellar populations, with some regions showing bluer hues, potentially indicative of more recent star formation. There may be a faint bar-like structure present in the central region. Finally, the system doesn't seem to be undergoing a major merging event, but there could be minor signs of disturbance in the disk, based on the asymmetries in it.
