The object presents as a relatively smooth galaxy, with a spheroidal morphology. There is little apparent dust or spiral arm structure. The color indices suggest a galaxy dominated by an older stellar population, indicated by the redder color. There is some disturbance in the galaxy, suggesting a recent interaction or merger, however, the galaxy does not appear to have a strong merging signature. The galaxy appears to be quite massive and exhibits a low rate of star formation. Overall, the galaxy appears to be a fairly evolved, quiescent system.
