The galaxy presents as a centrally concentrated object, with a morphology that is largely smooth and elliptical in appearance. The light distribution suggests an older stellar population, with a significant amount of light emitted in the redder wavelengths and lower levels of blue light emission. There is minimal evidence of distinct spiral arm structure, and the galaxy is likely a relatively quiescent system. There is also no evidence of a major ongoing merger, though a possible minor disturbance cannot be completely ruled out.
