The galaxy presents as a relatively smooth and centrally concentrated object. It displays an overall elliptical morphology, appearing mostly round with slight elongation. The core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. This core luminosity gradually diminishes towards the outer regions of the galaxy. Faint, diffuse extensions are visible surrounding the central area, suggesting a halo structure. There are some signs of minor disturbances or interactions. The redder colors indicate relatively low recent star formation activity. Based on these features, it is likely a mature galaxy with a substantial stellar mass.
