This galaxy exhibits an elliptical morphology, displaying a smooth, centrally concentrated light distribution. The galaxy is relatively elongated with a major axis extending further than its minor axis. The luminosity appears highest in the central region, gradually decreasing outwards. A subtle color gradient is observed, with the core appearing slightly yellower compared to the bluer hues in the outer regions of the galactic halo. No distinct spiral arm structures or significant dust lanes are visible, further supporting the elliptical classification. The overall appearance suggests a relatively evolved system.
