The galaxy appears to be undergoing a merger or interaction. Two distinct, roughly circular, light concentrations are visible, suggesting the presence of two galactic nuclei. The overall color of the galaxy is yellow/orange, possibly indicating an older stellar population with relatively low recent star formation. The galaxy appears relatively smooth overall, with high likelihood of being smooth, but also possibly showing some features due to the galactic interaction, but the image resolution limits detailed morphological analysis. There is a lack of any spiral arm structure detectable, which, given the system’s estimated distance, implies a relatively quiescent or elliptical morphology. Some tidal disturbances may be occurring, as it may have some visible asymmetric features, but overall the system is dominated by the two distinct centers of light. The brighter of the two components appears slightly larger.
