The galaxy presents a primarily smooth morphology, appearing as an elliptical-type system. There is a central concentration of light, suggesting a bulge component, surrounded by a more diffuse halo of stars and gas. The shape is roughly in between round and elliptical, with no obvious strong spiral arm structure or bar features. There may be subtle hints of tidal disturbances or minor asymmetries in the outer regions, but overall the galaxy appears relatively undisturbed. The color gradient indicates an older stellar population, especially towards the central regions, with the outer regions appearing somewhat bluer, implying ongoing star formation in those regions. The galaxy shows no strong evidence of a major ongoing merger event.
