The galaxy presents as a relatively smooth and centrally concentrated object. Its morphology appears largely elliptical, exhibiting a high degree of roundness. There is little evidence of spiral arm structure or significant disk features. A slight elongation can be observed, but the overall shape is predominantly spheroidal. The color appears to be somewhat redder. There are some signs of minor disturbance, but the galaxy appears mostly unperturbed, lacking strong tidal features or obvious signs of a major merger. The overall appearance suggests a mature system that has largely exhausted its gas supply and is no longer actively forming stars.
