The galaxy appears to be a relatively bright, face-on system, likely a lenticular or early-type spiral, exhibiting a pronounced central bulge that dominates its overall light profile. The bulge appears smoothly distributed with a high degree of spherical symmetry. Faint traces of what might be a disk component exist, but this is difficult to resolve and contains no visible spiral arms. The galaxy is moderately red, with a hint of ongoing or recent star formation, as evidenced by a subtle blue-green hue in the outer regions and a small amount of dust. A small tidal disturbance might be slightly disrupting the smooth outer halo of the galaxy.
