The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated brightness profile. A dominant, reddish core transitions to a more diffuse, bluer outer halo. The overall shape is generally round. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image. Based on the general undisturbed morphology, there is no strong evidence of a major ongoing merger. However, there is a slight possibility of minor tidal disturbances.
