This galaxy presents as a spiral galaxy, exhibiting well-defined, tightly wound spiral arms emanating from a central bulge. The morphology suggests a likely classification toward the later spiral types, potentially an Sc or Sd galaxy. The arms show signs of active star formation, indicated by regions of bluer coloration, likely tracing HII regions ionized by massive, young stars. The central bulge appears moderately sized, presenting a more yellowish or white hue in comparison to the arms. There is evidence of an ongoing or recent merger event. The galaxy shows clear signs of disruption. The spiral structure is distorted. A second galactic center can be observed. Based on the morphology, this galaxy likely has a moderate redshift and exhibits a significant amount of disk-like structure. There appears to be little to no bar structure.
