The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a high surface brightness, appearing as a concentrated luminosity. This central region is surrounded by a more diffuse halo of light, fading gradually into the background sky. There is an apparent elongation in the galaxy's shape, suggesting it is not perfectly spherical. No distinct spiral arm structures are visible. The galaxy appears to be relatively isolated, without any obvious signs of recent major mergers or tidal disturbances. Faint hints of bluer star forming regions are scattered through the galaxy. Overall, the galaxy appears to be relatively quiescent.
