The galaxy presents as a somewhat elongated, elliptical form. It exhibits a relatively smooth luminosity profile, with the brightest region concentrated towards the central bulge. The core is a prominent yellow color, indicating an older stellar population, while the outer regions appear fainter with hints of blue or green. This subtle color gradient could suggest ongoing, though perhaps limited, star formation in the outer parts of the galaxy. There does not appear to be evidence of strong spiral arm structures or significant dust lanes. No signs of a recent major merger are evident. Overall, the galaxy seems to be a relatively evolved system.
