The galaxy presents as a relatively smooth object. It exhibits a roughly elliptical morphology, appearing somewhere between round and slightly elongated. There is a central concentration of light that appears to be the galactic bulge. The overall color is a somewhat indistinct hue. This could indicate an older stellar population with lower ongoing star formation. There may be some minor tidal disturbances or asymmetries present, but without further information, it is difficult to be certain if these are signs of an interaction or merger. There are no clear indications of spiral arms or a prominent disk component.
