The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity from the core outward. The color appears to be bluish-white, suggesting a population of relatively young, hot stars or recent star formation. A subtle extension or tidal feature is observable extending from one side, potentially indicating a past or ongoing interaction or merger event. The galaxy exhibits a moderate degree of roundness. No obvious dust lanes or spiral arms are present.
