The galaxy presents as a relatively smooth, elliptical morphology with a high degree of roundness. There is a subtle color gradient, transitioning from a slightly bluer hue in the central region to redder tones in the outer halo, potentially indicative of differing stellar populations. No significant signs of disk-like structures or prominent spiral arms are apparent. The galaxy exhibits a slight asymmetry, possibly due to a minor gravitational interaction or disturbance. There are no obvious signs of a major ongoing merger. Overall, the galaxy appears to be a quiescent system, characterized by an older stellar population and low star formation rate.
