The galaxy presents as a relatively smooth, elliptical object. There is a concentrated, bright central bulge that fades into a more diffuse halo. The galaxy appears to be in a relatively undisturbed state, showing no signs of major mergers or significant tidal interactions. The color profile indicates the presence of an older stellar population, suggested by the yellowish-red hue. While some subtle variations in color intensity are observed, there are no distinct spiral arm structures or prominent star-forming regions discernible in the image. The morphology suggests a evolved system, possibly an elliptical galaxy with little ongoing star formation. 
