This galaxy presents as a largely smooth, elliptical morphology. The core exhibits a high degree of concentration, with a gradual decrease in luminosity outward. The galaxy displays a color gradient, transitioning from a yellow-white center to a redder periphery. No distinct spiral arms or dust lanes are discernible. There is some marginal evidence of minor tidal disturbance and a faint outer halo. The object’s overall shape is approximately round. Star formation appears to be relatively suppressed. The galaxy appears as a single, integrated structure, and no obvious signs of an ongoing major merger event are present, though there may be some minor gravitational interaction.
