The galaxy presents as a roughly elliptical, centrally concentrated structure. The core region exhibits a bright, yellowish-white hue, indicating a population of older stars. The luminosity gradually decreases outwards from the center. Surrounding this central bulge is a less distinct, fainter halo of bluish-white light. The galaxy appears relatively smooth, with no obvious spiral arm structures or dust lanes visible. The morphology suggests a minimal amount of active star formation and minimal signs of any ongoing mergers or disturbances. The overall form is consistent with an early-type galaxy, possibly an elliptical or lenticular. The spatial extent is relatively small, possibly corresponding to 5-6 kiloparsecs.
