The galaxy appears to be a relatively smooth, elliptical type, with a high degree of central concentration. The light is dominated by a yellowish hue, which is characteristic of older stellar populations. A slight elongation is visible, indicating that the galaxy is not perfectly spherical, but rather somewhat ellipsoidal. There is little evidence of spiral arms or distinct features associated with active star formation. A faint blue tinge is present, indicating some ongoing but low-level star formation. There are no signs of mergers or major tidal disturbances.
