This galaxy exhibits an elliptical morphology, appearing as a flattened spheroid. The central region displays a concentrated, bright core. The outer regions show a gradual decrease in luminosity, indicative of a smooth transition in stellar density. There is some evidence of a disk or arms. Color gradients are noticeable within the galaxy. The central bulge shows a redder hue, possibly due to an older stellar population. The outer disk regions display a bluer tint, suggesting ongoing star formation activity. There is a moderate degree of disturbance to the morphology.