The galaxy presents an elliptical morphology with a smooth, concentrated light distribution. The core exhibits a high surface brightness, appearing almost stellar, and suggests the presence of an active galactic nucleus (AGN) or a supermassive black hole. The galaxy displays a reddish hue, indicative of an older stellar population dominated by red giants and a suppressed rate of star formation. There is a subtle flattening observed, deviating slightly from a perfect circular shape. No distinct spiral arms or dust lanes are discernible within the observed wavelengths. The galaxy appears relatively isolated, without any clear signs of tidal interactions or ongoing mergers with nearby galaxies. The overall structure indicates a mature, evolved system, likely nearing the end of its star-forming epoch.
