The galaxy appears as a centrally concentrated object, exhibiting a smooth and relatively featureless morphology. The light profile indicates a high degree of central symmetry, showing a near-circular shape. There is no visual evidence of spiral arms, bars, or prominent dust lanes. The color gradient across the galaxy is subtle, suggesting a relatively uniform stellar population, with slight reddening towards the core. No significant signs of tidal disturbances or ongoing major mergers are apparent, suggesting a dynamically relaxed system. Faint indications around the primary body suggest a extended halo. The overall impression is that of an elliptical galaxy or a lenticular galaxy seen nearly face-on.