The galaxy appears as a luminous, centrally concentrated object, with a shape somewhere between round and elongated. The light distribution suggests a smooth morphology, lacking prominent spiral arms or significant irregular features. A slight color gradient is visible, with a more yellowish hue toward the central region that slowly fades to blue/white as we look away from the core, possibly indicating an aging stellar population. There is faint evidence of minor disturbances, with some possible tidal features in the outer regions of the galaxy. The galaxy does not appear to be undergoing a major merger, and no distinct dust lanes are discernible. Overall, the galaxy seems to be a relatively quiescent system.
