The galaxy presents a complex morphology, potentially indicating an ongoing or recent interaction. A dominant, smoother component is observed with an elliptical shape, suggesting an older stellar population. This primary component exhibits a general yellowish-white color. Juxtaposed to the primary component is another, smaller area with a bluer hue, which might indicate more recent star formation. There also appears to be some irregularities in the morphology, suggesting a possible tidal disturbance or ongoing merger event. A bridge of fainter material may connect these two components. The overall structure appears moderately diffuse, lacking a sharp boundary.
