The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that fades gradually into the outer regions. The color profile suggests a redder hue, indicative of an older stellar population and lower levels of current star formation. The round shape of the galaxy suggests it is likely a type E0-E3 galaxy. There appears to be a smaller object possibly interacting with the larger galaxy. There are no obvious signs of spiral arms or dust lanes within the visible spectrum. The overall structure suggests a relatively evolved galaxy that is not undergoing significant current merger activity.
