The galaxy presents as a slightly elongated, yellowish-white structure with a brighter central bulge. The galaxy appears largely smooth in texture, with some subtle hints of a disk-like structure. There seems to be some internal structure that could be the beginning of spiral arms, but they are poorly defined. The galaxy's overall shape indicates that it is somewhere between a disk and a spheroidal morphology. There may be indications of minor disturbances in the galaxy, like a slight asymmetry in the spiral arms. These minor disturbances may indicate the presence of star-forming regions, and they are likely the origin of the increased blue and red light emissions. The galaxy displays an apparent lack of strong star formation, and it likely has a supermassive black hole in the center.
