The galaxy presents as a generally smooth, centrally concentrated object with a slightly elliptical morphology. The core exhibits a strong emission signature, appearing as a bright yellowish-orange hue indicative of a population of older stars or potentially a central active galactic nucleus. The galaxy shows a more diffuse blue emission surrounding the core, which suggests the existence of a younger population of stars or recent star formation in the surrounding region. Faint disturbances may be present in the outer regions. The disk of the galaxy appears to be a mixture of old and young stars.