The galaxy presents an irregular morphology, suggestive of an ongoing or recent interaction or merger. There appears to be at least two distinct luminous components, both exhibiting a blue hue. These components are connected by a fainter bridge of light, potentially tidal debris resulting from gravitational interactions. The overall structure lacks a well-defined disk or spiral arms. The stellar population appears young, as indicated by the blue color. The lack of a prominent bulge suggests a smaller mass concentration in the center of each luminous component. Overall, the galaxy appears to be actively forming stars but has a relatively low mass.
