The galaxy appears to be a relatively smooth, early-type galaxy, possibly an elliptical or lenticular system. The central bulge is prominent and exhibits a yellowish-white hue, which is indicative of an older stellar population. A faint, diffuse halo surrounds the bulge. The disk is not clearly visible, but there are subtle color gradients, with a slight increase in bluer hues further from the center. This suggests some presence of younger stars in the outer regions, though star formation activity appears to be low overall. The galaxy displays a slight elongation, tending toward an elliptical shape rather than being perfectly spherical. There are some faint, possible disturbances in the outer regions, but no clear signs of an ongoing major merger.
