This galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population and potentially an active galactic nucleus. Moving outwards from the center, the luminosity gradually decreases. The galaxy's overall color appears yellowish-white, indicative of an older stellar population with fewer young, massive stars. The disk of the galaxy is not fully circular, appearing slightly elongated. There is no evidence of strong spiral arms or major tidal disturbances. Faint blue regions hint at localized star formation on the outer edges of the galaxy. 
