The galaxy presents as a faint, irregular structure with a dominant blue hue. Its morphology suggests an ongoing or recent interaction or merger event. There are noticeable bright knots of blue light, indicative of active star formation regions likely triggered by tidal forces or compression of gas clouds during the interaction. The overall form is elongated and disrupted, lacking a defined central bulge or spiral arm structure typical of more quiescent galaxies. The faintness of the galaxy suggests a relatively low mass and star formation rate, consistent with a dwarf galaxy undergoing morphological transformation. The tidal features may be disrupting the overall shape of the galaxy, creating an amorphous appearance. There is faint diffuse light surrounding the brighter star-forming regions, possibly indicating a more extended stellar halo associated with the merging process.
