The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggestive of a significant stellar population density, possibly around a supermassive black hole. Moving outward from the core, the light intensity gradually diminishes, displaying a diffuse halo surrounding the central region. There is evidence of a subtle disk-like structure, although it lacks prominent spiral arms. The color distribution appears relatively uniform across the galaxy, with a slight tendency towards redder hues, potentially indicating an older stellar population and reduced current star formation. There are also indications of minor disturbances in the outer regions, hinting at possible past interactions or mergers, but these features are not exceptionally pronounced.