The galaxy appears to be a luminous, elliptical-type galaxy at a considerable distance. Its overall morphology is smooth and largely featureless, with a centrally concentrated bulge. The core exhibits a bright, yellowish hue, possibly indicating an older stellar population or dust obscuration. The galaxy displays a high degree of circularity, with no obvious signs of a disk component or spiral arms. There is a subtle color gradient, with the outer regions showing a slightly bluer tint. Overall, the galaxy appears undisturbed, lacking significant tidal features or signs of recent merger activity. The overall light distribution is relatively even, suggesting a relaxed stellar configuration within a single, massive system.
