The galaxy appears as a centrally concentrated, relatively smooth structure. Its color suggests it is primarily composed of older stellar populations, exhibiting a reddish-yellow hue overall. There is little indication of spiral arm structure or significant dust lanes. The object's shape is neither perfectly spherical nor elongated, appearing as somewhere in between. There is no strong visual evidence of ongoing merger activity or major disturbances in its morphology, however there is a chance of minor disturbance.
