The galaxy presents a largely smooth morphology, appearing as a fairly regular elliptical or lenticular galaxy. The light distribution is concentrated towards the center, indicating a significant bulge component. The isophotes appear generally round. There is a subtle color gradient, with the central region exhibiting a slightly yellower hue compared to the outer regions, hinting at an older stellar population in the core. The overall color suggests an intermediate age population, without significant ongoing star formation activity. There is no obvious dust lane or spiral arm structure visible. Based on its characteristics, the galaxy appears to be relatively undisturbed, showing no signs of major merger events or significant tidal interactions.
