The galaxy presents as a disk-dominated system, seen at a significant inclination. It exhibits a notable central bulge component, appearing more concentrated and with a yellowish-orange hue, indicative of an older stellar population. Fainter spiral arm structures are discernible, appearing somewhat flocculent and blueish, suggesting regions of ongoing star formation. There is some evidence of minor disturbances within the disk, such as slight asymmetries or subtle tidal features. Overall, the galaxy seems to be in a relatively quiescent state.
