The galaxy presents a diffuse, somewhat amorphous structure. It exhibits a bluish central region, suggesting ongoing or recent star formation activity. The overall form is irregular, with no discernible spiral arms or defined bulge. There is evidence of some degree of disturbance in the galaxy's morphology. Faint wisps or extensions appear to emanate from the central region, indicating possible tidal interactions or recent merger events. The galaxy appears to be of relatively low mass.