The galaxy presents an elliptical morphology, appearing predominantly smooth with a high degree of central concentration. Its overall color is moderately red, suggesting an older stellar population and lower rates of ongoing star formation. The disk exhibits a notable inclination relative to our line of sight, displaying a somewhat elongated shape. There are no clear signs of a significant merger event or major tidal disturbances impacting the galaxy's structure. Faint, extended halos might be present but are not very apparent.
