The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution across the majority of its structure. The core region exhibits a brighter, more concentrated luminosity. A noticeable redder component is visible at what appears to be the lower extreme of the galaxy, suggesting either a region of older stellar populations or significant dust obscuration. There is a suggestion of some tidal feature or disturbance extending, with indications that the system might be undergoing some merger activity. A strong probability exists that it is a pre-merger system.
