The galaxy presents a generally smooth and centrally concentrated morphology. The light profile appears relatively featureless, lacking prominent spiral arms or a distinct bar structure. The overall shape is close to circular, showing only a slight deviation toward an elliptical form. A bright, yellow-white core dominates the central region, suggesting a significant concentration of older stars. The outer regions display a gradual fading in luminosity, exhibiting a diffuse, reddish-tinged halo surrounding the brighter core. There is no obvious evidence of tidal disturbances, major mergers, or active star formation regions within the observable structure of the galaxy. The galaxy appears to be an evolved system with limited ongoing star formation activity.