The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is a noticeable color gradient, transitioning from a yellowish-white core to a fainter, slightly bluer outer region. The galaxy exhibits a subtle degree of elongation, deviating slightly from a perfect circular shape. No distinct spiral arms or prominent dust lanes are visible within the observable structure. The overall structure suggests a relatively evolved system, potentially with a large stellar mass and a low star formation rate. There is no clear evidence of ongoing major mergers or significant tidal disturbances in the galaxy's immediate environment.