The galaxy exhibits a smooth, elliptical morphology. It displays a concentrated central bulge that appears to be older stellar populations, indicated by the yellowish-white hue. The galaxy has an elongated shape, appearing cigar-like. There is no clear evidence of spiral arm structure or significant dust lanes within the galaxy. Faint blue tinges on the outer edges suggest the presence of a small amount of younger stars. No signs of any major ongoing mergers are visible, however, there may be minor disturbances, or perhaps tidal features. The overall color suggests the galaxy's star formation rate is relatively low.
