This galaxy presents as a somewhat smooth, elliptical structure. The central region exhibits a concentrated, bright yellowish-white hue, suggesting a population of older stars. The light intensity diminishes gradually outward from the core. A slight elongation is observed, moving away from the central core in the vertical direction. The outer edges appear diffuse and less defined, transitioning into the background sky. There is no evidence of prominent spiral arms or significant dust lanes. The color gradient suggests possible ongoing, though limited, star formation at a relatively low rate within the galaxy. There is no obvious visual disturbance.
