The galaxy appears to be undergoing a merger event. There are two distinct nuclei, one appearing slightly more diffuse than the other, suggesting potentially different stages of tidal disruption or variations in stellar density. The overall morphology is irregular, lacking a defined spiral or elliptical structure. A faint blueish hue is present within the central region, which suggests ongoing or recent star formation. The galaxy exhibits a relatively compact size, spanning only a small portion of the image. A tidal tail or bridge is potentially visible, connecting the merging components but is not distinctly defined. Based on its apparent color and morphology, the galaxy is likely relatively active.
