The galaxy presents an irregular morphology, with a generally amorphous central region. There is evidence of disturbed morphology, potentially indicative of an ongoing or recent merger event. The galaxy exhibits a yellow-orange hue, suggesting an older stellar population with possible dust obscuration. The system's overall shape appears somewhat elliptical, but with clear deviations. There's possible presence of a faint tidal tail or arm-like structure extending from the main body, further supporting the merger hypothesis.
