The galaxy presents a largely smooth, elliptical morphology. It exhibits a high degree of central concentration, with a luminous core that gradually fades into a less distinct halo. The color profile suggests an older stellar population, with a redder hue in the central regions transitioning to slightly bluer tones in the outskirts. There is no evidence of prominent spiral arms, bars, or significant dust lanes. A slight asymmetry or minor perturbation might be present in the outer halo, though this is subtle. Overall, the galaxy appears to be relatively undisturbed, showing no clear signs of ongoing major merger activity or significant star formation.
