The galaxy appears as a relatively compact, smooth object. Its morphology suggests it is likely an elliptical galaxy with a high degree of sphericity. The color is predominantly bluish, indicating the presence of younger, hotter stars and ongoing star formation. There might be a slight disturbance in the light distribution, possibly indicating a minor interaction with another galaxy or internal dynamical processes. No obvious spiral arms or significant dust lanes are visible. The overall shape is quite regular, with a high degree of central concentration.
