The galaxy presents as a centrally concentrated spheroid, exhibiting a smooth, elliptical morphology. The core region displays a bright, yellowish hue, indicating a significant population of older stars. Moving outward, the light gradually fades, suggesting a diminishing stellar density towards the galaxy's periphery. There are no apparent spiral arm structures or significant dust lanes visible. The galaxy appears relatively undisturbed, showing no signs of ongoing mergers or major tidal interactions. The overall color profile suggests a relatively quiescent galaxy with a low rate of active star formation.
