The galaxy presents a generally smooth, elliptical morphology. Its color profile indicates a dominant population of older stars, exhibiting a yellowish hue centrally, transitioning to a slightly redder tinge towards the outer edges. There's little indication of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, showing no obvious signs of a recent major merger event. It exhibits a moderate degree of roundness. There are no prominent bright knots of star formation.
