The galaxy presents as a dominant, centrally located elliptical morphology, appearing largely smooth in texture. Its light profile shows a centrally concentrated luminosity, fading gradually toward its outer regions. The object exhibits a somewhat flattened shape, deviating slightly from a perfect circle. 

Based on the color indices derived from the image data, the galaxy's overall color is relatively red, suggestive of an older stellar population and a reduced rate of ongoing star formation. The galaxy appears to have a high stellar mass. There is no obvious indication of spiral arms, a bar, or recent major merger activity within the visible structure. Subtle asymmetries may exist in the outer regions, hinting at minor gravitational interactions or disturbances, though the primary structure remains well-defined.
