The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that fades outward into a more diffuse halo. The overall color is yellowish-orange, suggestive of an older stellar population. There's a slight asymmetry in the halo’s extension, possibly indicating a minor interaction or past merger event. No distinct spiral arm structure is visible, and it is consistent with a relatively inactive galaxy in terms of star formation.
