The galaxy presents a somewhat amorphous structure. It exhibits a central, moderately bright bulge that appears to be surrounded by a fainter, more diffuse halo. There is not a well-defined disk structure present. The morphology suggests this is likely a relatively evolved galaxy, transitioning towards an elliptical form. The central region shows a more concentrated and potentially older stellar population while the outer regions are much more diffuse. There are some slight disturbances to the structure of the galaxy that indicates it might be undergoing a minor interaction.