The galaxy appears as a single, relatively smooth and concentrated object. It exhibits a generally elliptical morphology, appearing mostly round. The light is concentrated towards the center of the galaxy, with intensity gradually decreasing towards the outer edges. Color gradients are subtle, but the core presents a warmer, yellower hue transitioning towards slightly cooler, redder tones at the periphery. There are no prominent spiral arm structures or dust lanes visible in the image. The overall appearance suggests a lack of significant ongoing star formation or major disturbances. The galaxy does not seem to be undergoing a major merger, though there may be a slight asymmetry that could indicate a minor interaction. 
