This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge that graduates into a more diffuse halo. The core region exhibits a yellowish hue, potentially indicating an older stellar population. There's a subtle transition into a bluish halo, hinting at younger, hotter stars in the outer regions, possibly indicating an ongoing, but relatively low level of star formation. The galaxy's overall morphology suggests it has not experienced recent major mergers, but there is a hint of asymmetry that could be due to a minor disturbance or past interaction. The galaxy presents a moderately round appearance in its shape. Overall, it seems to be a relatively massive galaxy with a mixed population of older and younger stars.
