The galaxy presents as a relatively compact object with an overall elliptical morphology. There is evidence of a central, bright region that is elongated in shape. A fainter, diffuse halo surrounds this central structure. The galaxy appears to be experiencing an ongoing merger. The color profile indicates a generally older stellar population, particularly in the central regions, with a hint of possibly younger, bluer stars located at the peripheries. There is visible disturbance of the galaxy which possibly indicates an interaction. 
