The galaxy presents as a centrally concentrated object with a smooth, symmetrical morphology. The core region exhibits a distinct yellowish-orange hue, suggesting an older stellar population likely dominated by evolved stars. Surrounding the core, a more diffuse, bluish halo extends outwards, indicative of some ongoing or recent star formation activity. The galaxy appears largely undisturbed, with no obvious signs of tidal features or major mergers. A slight asymmetry is noted in the outer regions of the halo, but this is not a clear indicator of an interaction. Overall, the galaxy seems to be a fairly well-evolved system with a mix of older and younger stellar populations.
