The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, indicative of a high stellar density and potentially a supermassive black hole at the center. The light profile suggests a fairly round shape. A faint, extended halo surrounds the central region, gradually diminishing in intensity with radial distance. There's a subtle color gradient, shifting from a more yellow-ish, potentially older stellar population at the core, to slightly bluer tones in the outer regions. The smooth texture implies it is unlikely undergoing a major merger, though minor disturbances cannot be ruled out due to the limited resolution.
