The galaxy presents as a moderately bright, elliptical-like structure. It exhibits a smooth, centrally concentrated morphology with a notable lack of distinct features such as spiral arms or prominent dust lanes. The light distribution suggests a relatively uniform stellar population. There appears to be a gradual decrease in luminosity from the core outwards, indicating a diffuse halo. Color gradients are subtle, with a possibly slightly redder core transitioning to bluer outer regions. Overall, the galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or mergers.
