The galaxy appears as a centrally concentrated object with a slightly elongated, elliptical morphology. The core exhibits a yellowish-white hue, suggesting a population of older stars. Progressing outward from the core, the galaxy transitions into a bluer color gradient, possibly indicating younger stellar populations or regions of ongoing star formation in the outer regions. The galaxy appears relatively smooth in texture, exhibiting no prominent spiral arm structures or significant dust lanes. The overall structure suggests a relatively evolved system that does not display major merger events, yet it may have minor tidal distortions. The galaxy has a relatively compact apparent size, its light distribution decreasing gradually from center. 
