The galaxy appears to be a relatively smooth, elliptical type, exhibiting a pronounced central bulge that gradually fades into a diffuse halo. The color profile suggests a dominant population of older stars, with a yellowish-orange hue concentrated in the core region. There are subtle variations in the surrounding halo, hinting at possible interactions or minor disturbances in its past, but the overall structure remains largely undisturbed. No prominent spiral arms or significant dust lanes are visible. The galaxy's shape is somewhat elongated, though not extremely so.
