The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a centrally concentrated, bright core that gradually fades outwards into a more diffuse halo. The overall color profile suggests a population of older stars, with a yellowish hue dominant throughout the galaxy. There is little evidence of spiral arms or distinct features indicative of active star formation. The galaxy's shape appears mostly round, with a slight deviation from perfect circularity. No obvious signs of ongoing or recent merger activity are discernible. The galaxy's size is relatively compact, and the light distribution seems fairly uniform, lacking significant clumps or substructures.
