The galaxy presents a primarily smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, indicating a significant population of older stars. The overall color appears yellow to orange, suggesting a lack of significant ongoing star formation. There is a subtle asymmetry in the outer regions of the galaxy. A faint, irregular structure extends outwards, potentially indicative of a minor interaction with another galaxy or past merger event. There is a hint of distortion in the disk, but it's hard to ascertain.
