The galaxy presents a predominantly bluish hue, suggesting ongoing or recent star formation activity. Its morphology appears irregular, lacking a well-defined spiral structure or elliptical form. There's a suggestion of a possible disk structure viewed at an oblique angle, but this is not clearly defined. The central region does not exhibit a prominent bulge. There seems to be some kind of disturbance, such as a tidal tail or the presence of distorted features, indicating a possible interaction or merger event.
