The galaxy presents as a centrally concentrated, smooth light distribution, generally elliptical in shape. There is no evidence of a prominent disk structure or spiral arms. The core region exhibits a bright, concentrated glow, transitioning outward to a more diffuse halo. The light appears yellowish, suggesting a population of older stars, although color gradients may be present. No significant morphological disturbances are apparent. There is a clear lack of any substantial dust lanes or patchy star-forming regions. The galaxy appears relatively isolated and undisturbed.
