The galaxy appears to be a smooth, centrally concentrated object, potentially an elliptical galaxy, exhibiting a roughly circular morphology. The color profile is dominated by yellowish hues, suggesting a stellar population that is old and redder. There is no apparent disk structure or spiral arms. The galaxy appears isolated, with no immediate signs of tidal interactions or ongoing mergers. The light is relatively evenly distributed without any sharp gradients, except toward the very center where the object brightens significantly, a possible indication of an active galactic nucleus. The lack of visible blue light implies a low rate of on-going star formation.
