The galaxy appears as a relatively smooth, elliptical-like structure with a high degree of central concentration. Its color profile suggests an older stellar population, with a dominant yellowish hue emanating from the core and inner regions. There's a gentle color gradient extending outwards, fading towards the edges with hints of redder tones, indicative of potentially cooler stars or dust absorption. There is a high degree of roundness. The overall morphology shows minimal signs of recent or ongoing major disturbances. Star formation is likely present at a low rate. The galaxy appears fairly massive. 
