The galaxy presents with an overall elliptical morphology. The central region exhibits a smooth, concentrated light distribution indicative of an older stellar population. The central bulge is an orangish-yellow color. Extending away from the core, one side of the galaxy is slightly more elongated and presents a bluish color. This may be suggestive of a tidal tail or distortion due to an interaction with another galaxy, or star formation in the galactic disk. There appears to be some disturbed structure. The galaxy is not perfectly round, appearing somewhat cigar-shaped. There may be a merger occurring.
