The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, fading into a diffuse halo. The color profile suggests a population of older stars dominating the light output, particularly in the bulge region, which appears more yellow/orange. There's little evidence of spiral arms or significant dust lanes. The overall structure appears relaxed and undisturbed, showing no signs of recent major mergers. There is some slight asymmetry visible in the outer regions of the halo. Based on its apparent roundness, it appears to be nearly face-on relative to our line of sight.
