The galaxy presents a predominantly smooth, elliptical morphology. The core region exhibits a concentrated, bright glow, suggesting a high stellar density, possibly indicating an older stellar population. This bright emission gradually diminishes outwards, transitioning into a fainter halo. The light appears reddish-orange, which may be due to redshift, indicative of the galaxy's recessional velocity. The overall shape is elliptical, with a moderate degree of roundness. There is some indication of a slight asymmetry or minor disturbance in the outer regions, but overall the galaxy appears relatively undisturbed. No strong evidence of spiral arms or significant disk features are visible. Based on the smooth and concentrated appearance, the galaxy is likely to be at a considerable distance.
