The galaxy appears to be a relatively smooth, elliptical system. It presents with a concentrated central bulge that exhibits a yellowish-orange hue, possibly indicating an older stellar population. Surrounding this central region is a more diffuse halo of light that graduates into a bluish-white color. The lack of distinct spiral arm structure or significant dust lanes suggests a classification toward the earlier end of the Hubble sequence, likely an E type. It seems to have intermediate roundness. There are no obvious signs of a recent major merger event, though some minor disturbances cannot be ruled out. The overall structure suggests a quiescent galaxy with a subdued star formation rate.
