The galaxy presents as a slightly elongated, elliptical-like structure with a smooth overall appearance. There is a subtle color gradient observed across the galaxy, with the central region appearing redder, potentially indicating an older stellar population. Moving outward from the core, the color shifts toward bluer hues, which may suggest regions of more recent or ongoing star formation in the outer parts of the galaxy. Despite the overall smooth characteristic, there are some signs of minor disturbances present in the disk of the galaxy, though it is not undergoing an ongoing or recent major merger. The galaxy has no distinct, organized spiral arm structure that is typically seen in barred or unbarred spiral galaxies.
