This galaxy presents as a fairly smooth, centrally concentrated object. The light distribution suggests a general elliptical morphology, although it deviates somewhat from a perfect ellipse, appearing slightly elongated. A noticeable color gradient is observed, transitioning from a bluer hue at the top to a redder hue at the bottom. This may indicate differing stellar populations and/or dust content within the galaxy. No distinct spiral arms or prominent star-forming regions are apparent. The galaxy exhibits a slight asymmetry, possibly hinting at a minor gravitational disturbance or interaction.
