The galaxy presents as a centrally concentrated, elliptical-like structure. The core region exhibits a bright, yellowish hue, indicative of an older stellar population. The light gradually fades with increasing distance from the center, suggesting a smooth density gradient in the stellar distribution. No distinct spiral arm structures or dust lanes are visible. The overall morphology appears relatively undisturbed, with no obvious signs of ongoing major mergers or significant tidal interactions. A slight asymmetry is observed in the outer regions, potentially indicating a minor disturbance or past interaction. The color profile suggests a relatively quiescent galaxy with low rates of current star formation.
