The galaxy appears as a single, relatively smooth and rounded object. The central region exhibits a concentrated and bright yellowish-white glow. This suggests a significant population of older stars and potentially a supermassive black hole actively accreting material. The outer regions of the galaxy display a gradual fading of light, transitioning into a more diffuse reddish hue, possibly due to a lower density of stars and an increased presence of dust absorbing bluer wavelengths. The overall shape is nearly circular with no discernible spiral arms or bar structures. The object appears largely undisturbed, exhibiting no significant signs of tidal interactions or ongoing mergers. 
