The galaxy presents as a fairly smooth, elliptical structure, with a centrally concentrated, bright core. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central regions. The outer regions show a slight decrease in intensity, fading smoothly into the background. There's a very subtle bluer tint to the outermost edges of the galaxy, which could indicate some residual star formation, but overall, the galaxy lacks prominent spiral arm structures or intense blue star-forming regions. Its shape appears moderately elongated, not perfectly spherical, trending towards a disk-like appearance, though without any well-defined features. There is no visual indication of any major ongoing merger events, although subtle disturbances are possibly present.
