The galaxy presents as a primarily smooth, elliptical-like structure. The central region exhibits a concentrated, yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a bluer tint, possibly indicating a presence of younger, hotter stars or perhaps some residual star formation. The overall morphology is somewhat elongated, deviating slightly from a perfect sphere, and could be classified as somewhere in-between round and cigar-shaped. There's no visually prominent spiral structure or distinct disk component visible. Minimal signs of tidal disturbances or major mergers are apparent. Any minor disturbances, if present, are subtle. The galaxy appears relatively isolated and self-contained in the image, and the degree of star formation is low.
