The galaxy presents a largely smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, appearing mostly round, and appears to have a relatively large effective radius. Its color profile suggests a population of older stars, as evidenced by its redder hue. There may be some signs of gravitational disturbance, though the main body remains largely intact. The light distribution is relatively smooth, suggesting a lack of significant dust lanes or spiral arm structures. Some irregular features are observed, possibly resulting from a merger event. Overall, the galaxy appears to be a quiescent, massive system with little on-going star formation.
