The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The galaxy exhibits a yellowish-white hue, indicative of an older stellar population, with redder light concentrated in the center. There is no distinct disk or spiral arm structure apparent in the image. The galaxy appears fairly isolated, without any obvious signs of recent major merger events or tidal disturbances, with the galaxy exhibiting a degree of symmetry, lacking significant morphological irregularities. There is a subtle extension or faint halo of light surrounding the main body of the galaxy.
