The galaxy presents as a single, concentrated body of light with a smooth, elliptical morphology. There is a bright central bulge that gradually diffuses outward, indicating a decreasing stellar density with radial distance. Coloration appears to be relatively uniform across the galaxy, suggesting an older stellar population. No distinct spiral arm structures or prominent dust lanes are apparent. Slight asymmetry may be present, though it is difficult to discern with certainty. The lack of observable substructure indicates a relaxed system which is not undergoing a major merger. 
