The galaxy presents as a centrally concentrated spheroid with a smooth, relatively featureless profile. The core exhibits a pronounced yellow-orange hue, suggesting a population of older stars. The isophotes appear largely elliptical, showing minimal deviation from a regular shape. There is no evidence of spiral arm structure or significant dust lanes. The outer regions exhibit a gradual decline in surface brightness, transitioning to a faint, diffuse halo. There are no obvious signs of recent major mergers or tidal disturbances. The overall morphology suggests a galaxy with a high degree of dynamical relaxation, consistent with an early-type classification, such as an elliptical galaxy.
