The galaxy presents an elliptical morphology, appearing largely smooth and relatively featureless. The central region exhibits a concentrated, bright yellowish-white glow, suggesting a higher density of older stellar populations. Moving outwards from the center, the color subtly shifts to a redder hue, which might indicate the presence of a population of cooler, older stars. The overall shape appears to be somewhat elongated. There is little evidence of strong spiral arm structures or significant dust lanes within the observed image, reinforcing the characterization as an elliptical galaxy. There is a possible minor visual disturbance to the galaxy on its left side, but this could be attributed to a light artifact. 
