The galaxy presents as a somewhat smooth, elliptical structure. The central region exhibits a high concentration of luminosity, suggesting a dense stellar population and potentially a supermassive black hole actively accreting matter. The galaxy appears nearly round, with only a slight deviation from perfect circularity.  Evidence of a disk-like structure is not prominently observed, but very faint features or arms cannot be fully ruled out due to the limited resolution. The galaxy displays a color gradient, shifting from a brighter white-yellow core to a more subtle blue-tinged outer halo. No clear signs of ongoing major mergers or significant tidal disturbances are readily apparent in the image. Faint, minor irregularities may be present in the outer regions, but these could be attributable to lower resolution or potential minor interactions. It appears relatively isolated within its immediate vicinity.
