The galaxy presents as a diffuse, centrally concentrated object. Its morphology is generally smooth with a near-spherical, elliptical-like shape. There is no discernible spiral arm structure or significant dust lane obscuration evident. The light is concentrated in a very compact core, which has a yellowish hue, with a gradual fading into the extended halo. There is only a hint of possible minor disturbance or faint tidal features, which are subtle and do not indicate a recent major merger event. Based on its colour, the galaxy has a mixture of older stellar populations, with possibly some ongoing star formation.
