The galaxy appears as a smooth, elliptical-like structure. The central region exhibits a bright, concentrated luminosity, indicating a dense stellar population and potentially a supermassive black hole actively accreting material. The light profile fades gradually towards the outer regions, with a diffuse halo seemingly devoid of distinct features like spiral arms or prominent dust lanes. The overall color suggests an older stellar population, with a dominance of redder wavelengths. There is no apparent evidence of significant ongoing star formation. The galaxy's shape is more rounded than elongated, displaying an intermediate ellipticity. There is no strong visible indication of any tidal disturbances or ongoing mergers with other galaxies.
