The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge and a gradual decrease in luminosity outwards. The color gradient suggests an older stellar population, with a yellowish hue dominating the galaxy's core. There is some evidence of a faint disk. There is an interacting galaxy on the left of the image, which presents a blue color, indicating the presence of ionized gas and active star formation. It appears disturbed and distorted, potentially from gravitational interactions with the larger galaxy. The system is likely undergoing a minor merger event.
