The galaxy appears to be a relatively smooth, elliptical galaxy, possibly at a considerable distance. Its central region is bright and concentrated, exhibiting a yellowish-orange hue, indicative of an older stellar population. The galaxy lacks any readily discernible spiral arm structure or significant dust lanes. There is a subtle color gradient, with the outer regions becoming slightly redder, which may indicate a decline in recent star formation activity. Its overall morphology suggests it is a well-formed, mature system, likely in a relatively quiescent state. No signs of active galactic nuclei or tidal disturbances are immediately apparent in this image.
