The galaxy appears to be an elliptical galaxy with a smooth, diffuse profile. It is centrally concentrated with a bright core, which fades gradually into a less luminous halo. The galaxy exhibits a noticeable red-orange hue in its central region, which transitions to a more bluish-green color in the outer regions. Its morphology seems to be more elongated than circular. There is a hint of possible disturbance, but the galaxy's overall structure suggests it is not currently undergoing a major merger. The galaxy displays evidence of ongoing low-level star formation.
