The galaxy presents a somewhat elliptical morphology, with a dominant, smooth bulge component. There is a subtle indication of a disk, but the bulge dominates the overall structure. The color gradient suggests a more evolved stellar population within the central region, appearing redder, while the outer regions exhibit a bluer hue, potentially indicating ongoing or recent star formation. The galaxy exhibits signs of a potential interaction or disturbance, possibly from a minor merger event which explains the relatively bright color. There seems to be no signs of strong star formation, which is reflected by the color and morphology of the galaxy. 
