The galaxy presents as a roughly elliptical structure, appearing mostly smooth with a slightly elongated morphology. The central region exhibits a concentrated luminosity gradient. There is a notable color gradient transitioning from a yellowish-white core to a slightly bluer halo. The outer regions show some faint structural features, possibly indicative of a disk or spiral arms, but these are not clearly defined. The general appearance indicates a relatively evolved system, potentially in the process of transitioning from active star formation to a more quiescent state. The overall color suggests an older stellar population, though some residual star formation might still be occurring. There's no obvious indication of significant interaction or recent merging activity, though minor disturbances might be present.
