The galaxy presents as an elliptical or lenticular type. It exhibits a relatively smooth, centralized luminosity profile. Coloration suggests an older stellar population, exhibiting a yellowish-orange hue concentrated toward the core. There is a slight flattening; it appears mostly circular but not perfectly so. No distinct spiral arms or significant dust lanes are visible. Faint, subtle irregularities in the outer regions may indicate minor past gravitational interactions, although the overall structure appears largely undisturbed. The galaxy's radial extent is relatively compact.
