The galaxy presents as a relatively smooth, rounded object, potentially of elliptical morphology. There is a slight elongation, but generally lacking strong disk features. The light distribution is centrally concentrated, with a gradual fading towards the outer regions. The color profile appears rather uniform, with a tendency towards the redder end of the spectrum and a concentration of yellow light near its center. There is no clear evidence of spiral arm structure or significant dust lanes. There appears to be little ongoing star formation. The overall structure is fairly undisturbed, with no obvious signs of recent major merger activity, although a minor disturbance cannot be ruled out.
