The galaxy presents a somewhat amorphous structure, appearing largely smooth and lacking distinct spiral arms or a well-defined bar. The central bulge region exhibits a high degree of luminosity, suggesting a substantial concentration of stars. There is a slight blueish tint to the outer regions, possibly indicating more recent star formation. The overall morphology hints at a disk galaxy with possible features, though these are faint, with perhaps minor disturbances present in the surrounding area. It does not appear to be undergoing any major merging events based on its shape.
