The galaxy appears as a generally smooth, centrally concentrated object, exhibiting an elliptical morphology. A slight elongation is visible, suggesting it deviates somewhat from a perfectly spherical shape. The core exhibits a bright, yellowish-orange hue, possibly indicating an older stellar population. A faint, diffuse halo extends outwards from the central region, with subtle hints of bluer colorations at the periphery, perhaps indicative of younger stars or ongoing, low-level star formation within that region. There is no obvious evidence of spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent major mergers.
