The galaxy appears to be a relatively bright, single object with a smooth, elliptical morphology. It exhibits a concentrated central bulge that decreases in intensity towards its outer edges. The color profile suggests a dominant population of older stars, indicated by the yellow-red hue of the light emitted. No distinct spiral arms or dust lanes are visible. There is a possible indication of minor tidal disturbances, though these are subtle, possibly indicating an ongoing or past interaction with a smaller companion.
