The galaxy presents as a roughly elliptical, disk-like structure, seen at an oblique angle relative to our line of sight. A central bulge region is visible, appearing as a concentrated area of high luminosity. The light distribution appears relatively smooth throughout the galaxy. There's a slight indication of a disk structure beyond the bulge, with some hint of spiral arm morphology, or at least some uneven distribution of luminosity. The color is mostly in the blue-green range, with a hint of a faint red shift on one side of the disk. The overall form is consistent with that of a disk galaxy, with a low rate of star formation. It is possible there is a very minor merger or disturbance event occurring.
