The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a bright, yellowish-white glow, suggesting an older stellar population dominates the central region. There appears to be a slight elongation in the galaxy's overall shape, deviating from a perfectly circular form. The outer regions of the galaxy show a gradual fading in intensity, transitioning into a more diffuse halo. There is little evidence of distinct spiral arms or significant dust lanes, further supporting its classification as an elliptical galaxy. The smoothness of the light distribution indicates a well-mixed stellar population and a relatively quiescent star formation history. Subtle color gradients are observed, with the core appearing more yellow compared to the outer regions, which exhibit a slightly redder hue. This could signify variations in stellar age and metallicity throughout the galaxy. Overall, the galaxy appears to be a mature and relatively undisturbed system.
