The galaxy presents as a moderately bright object with a slightly elongated, elliptical morphology. It appears relatively smooth in texture, lacking prominent spiral arms or a central bar. The color gradient suggests a higher concentration of older stellar populations within the central bulge, exhibiting a yellowish hue, while the outer regions are bluer, implying ongoing star formation activity, though it seems mild. The overall structure suggests a galaxy transitioning towards a more quiescent state. There are no obvious signs of recent major merger events or significant tidal disturbances.
