The galaxy presents as a relatively smooth, centrally concentrated object. The core exhibits a bright, yellowish hue, possibly indicating an older stellar population or the presence of an active galactic nucleus, although the resolution is insufficient to confirm the latter. Surrounding the core is a more diffuse, fainter halo of light, showing hints of a slightly flattened or elliptical morphology. There may be some subtle color variations within the halo, potentially suggesting regions of differing stellar populations. The general appearance indicates a relatively evolved system, likely with low ongoing star formation. There are no obvious signs of strong tidal disturbances or interactions with other galaxies in the immediate vicinity.
