The observed galaxy presents a morphology that appears largely smooth and spheroidal in nature. A central bulge region of relatively high surface brightness is evident. There are also red tinges and other colours around the bulge region that are consistent with a relatively low star formation rate. There appears to be some minor disturbance in the structure of this galaxy. It is not a strong disturbance, but it is there. A very slight tidal tail may be present. Overall, the galaxy does not appear to be undergoing a major merger event.
