The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of luminosity, appearing bright yellow and somewhat diffuse. Moving outwards from the core, the light gradually fades, transitioning to a reddish-orange hue. There is very little evidence of spiral arms or distinct features such as dust lanes. The shape deviates slightly from being perfectly round, leaning slightly towards a more elliptical form. There is no apparent sign of a major ongoing merger, although subtle distortions could indicate minor gravitational interactions. The galaxy appears to be an evolved system with a substantial stellar mass and relatively low levels of active star formation.
