The galaxy exhibits a disturbed morphology, indicating a likely ongoing or recent interaction with another galaxy. There are no clearly defined spiral arms or a central bar structure. The light distribution suggests an overall elliptical shape, but this is disrupted by a prominent region of intense blue emission, suggesting active star formation in that area. The presence of both blue and red-shifted emission regions within the galaxy's profile hints at complex internal dynamics, which are probably caused by merging or tidal forces. The bulk of the galaxy appears relatively smooth. The redder emission regions are likely older stellar populations.
