The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. It appears to be an elliptical galaxy, exhibiting a prominent bulge with a diffuse halo. The color gradient suggests a concentration of older stellar populations towards the center, indicated by the yellowish hue. The outer regions show a hint of blue, potentially from a younger, though subdued, stellar population. No distinct spiral arms or prominent dust lanes are visible. There is no clear indication of a recent or ongoing major merger event. It is a galaxy of substantial mass with a moderate amount of star formation.
