This galaxy exhibits a morphology suggesting a possible ongoing or recent interaction. The overall form is elongated, with a central bulge that appears less defined than a typical elliptical galaxy. The galaxy is relatively faint, with a blueish hue that is brightest in the center, suggesting active star formation in the core region. However, the overall color distribution is not uniform and it appears clumpy. Some regions are more blue, and others are more red, which would imply variations in stellar population and/or dust obscuration. The structure seems disturbed, with no clear spiral arm structure or well-defined disk evident. There's an irregular tail, which may be evidence of gravitational disruption due to a past interaction or merger event. The galaxy shows hints of tidal features in the outer regions. The faintness of the galaxy indicates that the object may be more distant, or that it is a low luminosity object.
