The galaxy presents as a single, centrally concentrated object with a smooth light profile. Its overall morphology appears largely spheroidal, with no obvious spiral arm structures or a prominent disk component visible in this image. There are very subtle hints of an extended stellar halo. The core is considerably brighter in the G and R bands, and then it fades into the Z band. Color gradients within the galaxy are subtle, suggesting a relatively uniform stellar population or well-mixed dust distribution. The galaxy appears undisturbed, showing no signs of ongoing major mergers or tidal interactions. There are hints of possible minor disturbances, but that is not fully clear. The structure is compact and lacks significant asymmetry.
