The galaxy presents as a largely featureless, smooth object. Its overall shape appears to be elliptical or spheroidal, with a high degree of roundness and no discernable disk-like structure. The central region exhibits a concentration of light, possibly indicating a galactic nucleus or a dense stellar population. There is a color gradient across the galaxy; it exhibits a relatively blue hue in the outer regions, transitioning to a redder or yellow hue toward the center, which could indicate older stellar populations concentrated in the core and ongoing star formation in its outer disk. There are no obvious signs of ongoing mergers or tidal disturbances affecting the morphology. Based on its characteristics, the galaxy is likely a passive, early-type galaxy, specifically an elliptical galaxy with a calculated distance of approximately 2 billion light years.
