The galaxy appears as a somewhat diffuse object with an overall elliptical morphology. It has a bright, concentrated central region. The light distribution appears relatively smooth, with a subtle fading gradient from the core outwards. The central region exhibits a bluish hue. There are potential signs of minor disturbance or tidal features evident in the light distribution, particularly a faint elongation or asymmetry extending from the main body of the galaxy. No clearly defined spiral arms or a distinct disk component are observed. There are signs of a merger in process, with an asymmetrical shape.
