This galaxy appears to be undergoing a merger or interaction. The main body exhibits a somewhat amorphous shape, lacking the distinct spiral arms of a grand design spiral galaxy or the uniform elliptical shape of an elliptical galaxy. There is evidence of possible tidal disturbances or streams of material extending from the primary body.

Two central bright areas are visible, suggesting the presence of two galactic nuclei, consistent with a merger event. One core is brighter than the other. The overall color is shifted toward the blue end of the spectrum, indicating a relatively younger stellar population and active star formation regions within the galaxy. The galaxy's light is more condensed in the center and dispersed toward the edges.
