The galaxy presents as an elliptical morphology, approximately 4 kpc in radius. Its structure is largely smooth, exhibiting a central bulge with a high degree of symmetry. The galaxy has a disk which is observed nearly edge on, but is disturbed. Color gradients suggest a population of younger, bluer stars within the disk. There is a distinct lack of any tidal features and no obvious signs of on-going major mergers, though it is difficult to ascertain minor merger activity due to the galaxy's distance and the image's resolution.
