The galaxy presents as a centrally concentrated object, roughly elliptical in shape. The core exhibits a bright, yellowish-white hue, potentially indicative of an older stellar population and/or active galactic nucleus activity. Proceeding outwards from the center, the color shifts to a more reddish-orange. This might suggest a transition to a region with ongoing or recent star formation within the galaxy. A faint greenish halo is present, particularly on the outer edges. This halo structure might indicate the presence of ionized gas or a younger stellar population undergoing active star formation. The galaxy appears relatively smooth in overall texture with no major disturbances or tidal tails apparent in this imaging. It seems to exist as a fairly isolated system.