The galaxy presents as a single, relatively compact object. Its light profile appears smooth and centrally concentrated, exhibiting a high degree of symmetry. The dominant color is a yellow-orange hue, suggesting an older stellar population with a reduced amount of ongoing star formation. There is no visual evidence of spiral arms or a distinct disk structure. The galaxy's morphology aligns with that of an elliptical galaxy or a lenticular galaxy viewed face-on. There are no obvious signs of tidal disturbances or ongoing mergers. 
