The galaxy exhibits a distinct spiral morphology, with prominent, well-defined arms emanating from a central bulge. The spiral arms appear to be relatively tightly wound. Two spiral arms are seen. The bulge itself appears relatively moderate in size compared to the overall galactic disk. There's evidence of a possible bar structure, although not particularly strong. The overall appearance is of a galaxy undergoing active star formation, as suggested by the luminosity. The image indicates that it is not currently undergoing a major merger, but there are indications of minor tidal disturbances that might be influencing the observed morphology. The color index suggests an intermediate type spiral galaxy.
