The galaxy appears as a centrally concentrated object with a smooth, diffuse profile. The light distribution suggests an elliptical morphology, exhibiting a gradual decrease in surface brightness from the core outwards. There is a hint of a flattened, disk-like structure although the image appears largely spheroidal. Color gradients are subtle, with a somewhat redder hue towards the central region, possibly indicating an older stellar population or increased dust obscuration. Peripheral regions display a fainter, bluer color, potentially indicative of more recent star formation. There does not appear to be significant disturbance or tidal features in the surrounding halo, suggesting it has not recently undergone any major mergers or interactions.
