The galaxy appears to be elliptical in shape, presenting a smooth, centrally concentrated luminosity profile. There is a distinct color gradient, with the core exhibiting a more yellow-orange hue that transitions to a greenish-yellow in the outer regions. This suggests a possible variation in stellar population or dust content across the galaxy. No prominent spiral arms or bar structures are discernible. There is no visually apparent tidal debris or other indications of recent major merger activity.
