The galaxy presents as a predominantly smooth, elliptical structure with a slightly elongated morphology. The central region exhibits a high concentration of light, appearing as a bright, yellowish core which indicates a population of older stars. The outer regions of the galaxy display a gradual decrease in surface brightness, extending into a fainter halo. There is some subtle color variation with possible dust lanes or regions of younger stars. The overall form suggests a relatively evolved system, but the slight irregularities and color variations indicate potential minor interactions or ongoing low-level star formation processes. Given the apparent size and the features observed, this appears to be a massive galaxy.
