The galaxy presents as a centrally concentrated, elliptical structure with a smooth luminosity profile, indicative of an early-type galaxy. The core appears bright, and a gradual decrease in light intensity extends outward. The color is predominantly yellowish-orange suggesting an older stellar population with minimal ongoing star formation. There is no discernable spiral arm structure or dust lanes within the galaxy's visible extent. Based on observed structure, the galaxy does not appear to be significantly disturbed by any major gravitational interactions.
