The galaxy exhibits a morphology consistent with an ongoing or recent merger event. Two distinct luminous regions are visible, suggesting the presence of two galactic nuclei in close proximity. These regions display a yellowish-white color, possibly indicating an older stellar population or dust obscuration. Faint tidal features or diffuse emission are observed extending from the primary regions. This suggests gravitational interaction and disruption of the galactic structures. The overall shape is irregular and elongated, deviating significantly from a typical elliptical or spiral morphology.
