The galaxy presents a disturbed morphology, characterized by a somewhat elongated and asymmetrical shape. The light distribution appears uneven, suggesting a recent or ongoing interaction. There is evidence of tidal features and potential ongoing merger activity. 

The overall color is consistent with an older stellar population, though some bluer regions, which may indicate younger star formation, can be seen. The galaxy is not perfectly smooth and shows signs of internal structure, further supporting the presence of disturbances.
