The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, appearing quite round. The light profile is diffuse with a gradual fall off in intensity from the center outwards. There is a brighter, almost stellar-like nucleus that is surrounded by a more diffuse halo of light. The color appears to be generally redder, indicative of an older stellar population. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy displays no obvious signs of interaction or merging. The structure appears largely undisturbed.
