The galaxy presents as a system with an elliptical morphology. The light distribution is centrally concentrated, with a smooth and gradual decrease in surface brightness outwards from the core. The core region appears relatively luminous and compact. The overall color of the galaxy is slightly redder in the central regions, transitioning to a bluer hue further out. There is no prominent disk structure, or spiral arm features visible, though some slight features are present. The galaxy appears relatively isolated, without any strong signs of tidal interactions or recent merger events. 