The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears to be tending towards elliptical, with an approximate effective radius estimated around 9 kpc. The galaxy is not perfectly spherical but tends towards roundness. There is a color gradient visible, with a yellowish central bulge and a slightly bluer outer halo. There is no distinct spiral arm structure visible; however, a very faint, disturbed disk may be present. There is no evident major ongoing merger activity and appears to be a relatively isolated object. The low levels of recent star formation suggest the stellar population is dominated by older, redder stars.
