The galaxy presents as a somewhat compact object, with a bright, concentrated core region dominating its overall appearance. The central region exhibits a bluish hue, suggesting the presence of younger, hotter stars, or potentially a strong contribution from ionized gas emission. Moving outward from the core, the light becomes more diffuse, and the overall color shifts towards a greener-yellowish tint, indicating a population of older stars and dust absorption of the bluer wavelengths. There is a faint hint of asymmetry, with perhaps a minor disturbance or irregularity in its morphology. It appears largely spheroidal in shape.
