The galaxy presents as a somewhat elongated, elliptical morphology. The central region exhibits a concentrated, brighter luminosity, suggestive of a dense stellar population or active galactic nucleus. The light is most likely redshifted towards the redder end of the spectrum. The outer regions appear fainter and more diffuse, fading gradually into the background sky. Faint, wispy features hint at a possible disk structure, although it is not clearly defined. There is a hint of minor disturbance, but no clear merging. Overall, the galaxy appears relatively smooth in texture with a relatively large mass and low star formation rate.
