The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile, with a high degree of central concentration. The light distribution appears largely symmetrical and rounded. There is no readily apparent substructure, such as spiral arms, bars, or dust lanes. The color profile suggests a centrally concentrated luminosity, transitioning from a more yellow hue in the core to a slightly redder color towards the outskirts. There are no visual signs of any major ongoing merger activity or tidal disturbances, with no prominent tidal tails or distorted isophotes visible. The apparent lack of blue emission indicates a comparatively low rate of current star formation.
