The galaxy presents a generally elliptical morphology, appearing somewhat flattened along its minor axis. It exhibits a smooth, concentrated central bulge that transitions into a more diffuse halo. The core region is characterized by a bright, yellowish-white emission, indicating a concentration of older stellar populations. The outer regions of the galaxy exhibit a fainter, reddish hue. There is little evidence of distinct spiral arm structures or significant dust lanes. Overall, the galaxy appears to be a relatively evolved system with a significant spheroidal component and minimal ongoing star formation.
