The galaxy appears as a faint, diffuse object with a somewhat irregular morphology. There is a subtle central concentration of light, suggesting a possible bulge component, although it is not well-defined. Some faint extensions or tidal features appear to be present, hinting at possible past interactions or ongoing disturbances. The overall color is somewhat blueish, which could indicate a degree of ongoing star formation, although this is difficult to confirm given the image quality. The galaxy does not exhibit a clearly defined spiral structure, nor does it appear to be a perfectly smooth elliptical. It is likely a low mass galaxy. The system may be undergoing some form of interaction or disturbance. Additional higher-resolution imaging and spectroscopic data are needed to determine with higher confidence its morphological type, star formation rate, and the nature of any tidal features.
