The galaxy presents a flattened, elliptical morphology. Its central region exhibits a concentrated luminosity, appearing yellowish-white, suggesting a relatively older stellar population. The galaxy's light gradually diffuses outward from the core. The outer regions display a bluer hue, implying the presence of younger, hotter stars, potentially indicating ongoing star formation. While the overall structure appears relatively smooth and undisturbed, there is a slight asymmetry, with one side extending further than the other. No distinct spiral arms or bar structures are discernible. The galaxy's color indices imply that it is moderately luminous, likely a massive galaxy with substantial stellar mass.
