The galaxy presents an elliptical morphology, appearing largely smooth with a central concentration of light. The core exhibits a yellowish hue, suggestive of an older stellar population dominating the central region. The outer regions of the galaxy show a gradual decrease in luminosity with a hint of bluer light on the periphery, possibly indicating the presence of younger stars in that region. The overall shape tends towards round, with no obvious signs of strong tidal interactions or major disturbances to its structure. There is a potential minor disturbance or structure in the lower left of the image, but it is not conclusive of any major interactions or merger events. The galaxy’s color profile indicates a presence of both older and younger stars with a dominant older population in the center. 
