The galaxy presents a primarily smooth, elliptical morphology, showing a spheroid-dominated structure. There is some evidence of a disk component with hints of spiral structure visible, although it is not sharply defined. The bulge region exhibits a yellowish color, which may indicate an older stellar population, while the disk shows bluer tones. This suggests ongoing or more recent star formation in the disk region. The galaxy exhibits an overall intermediate roundness in shape. There appears to be minor asymmetry or tidal disturbances, but it does not appear to be undergoing a major merger. Overall, the galaxy appears to be relatively undisturbed.
