The galaxy exhibits a morphology suggestive of an ongoing or recent merger. The system displays a disturbed structure, with two distinct luminous components. The primary component appears more concentrated, exhibiting a yellowish-red hue, possibly indicating an older stellar population or dust obscuration. The secondary component is more diffuse and elongated, appearing bluer in color, suggesting a younger stellar population and ongoing star formation. There is evidence of tidal features, potentially indicating gravitational interactions with a companion galaxy. The morphology indicates the system is not a pure elliptical or spiral. Overall, the galaxy appears to be dynamically active, displaying evidence of ongoing star formation and potential merger activity.
