The galaxy presents as a centrally concentrated, elliptical-like system, exhibiting a smooth overall morphology. The core region displays a bright, yellowish-orange hue, suggesting an older stellar population. A subtle color gradient is observed, transitioning towards a greenish-blue tinge in the outer regions of the galaxy's halo, possibly indicating the presence of younger, hotter stars or some level of ongoing star formation, though limited. The galaxy appears to be relatively undisturbed, with no prominent signs of tidal interactions or major mergers. It presents as somewhat flattened, and fairly compact object.
