The galaxy presents as a slightly elongated, lenticular or elliptical morphology. The central bulge exhibits a pronounced, concentrated luminosity, with a color profile suggestive of an older stellar population. The disk component, while present, is not sharply defined, showing a more diffuse and fainter distribution of light extending outward from the central bulge. There's a subtle color gradient noticeable, with the outer regions appearing marginally bluer, potentially indicating the presence of younger stars or ongoing star formation activity, though at a low rate. Overall, the galaxy appears relatively undisturbed, with no prominent signs of ongoing major mergers or tidal interactions. The morphology suggests a relatively high stellar mass. The smooth appearance indicates a galaxy that has largely completed its morphological transformation.
