The galaxy appears to be a relatively smooth, elliptical system. Its overall color profile skews towards the redder end of the spectrum. There is a concentration of yellow and red light toward the galaxy's center, suggesting an older stellar population. The light fades gradually towards the edges. The galaxy is very nearly round, and shows no evidence of spiral arm structure or significant dust lanes. There are no obvious signs of ongoing merger activity or major tidal disturbances. The galaxy presents a largely undisturbed morphology.
