The galaxy presents as an elliptical or lenticular morphology, appearing largely smooth and featureless. The light distribution is centrally concentrated, exhibiting a radial gradient decreasing in intensity towards the outer regions. The core exhibits a yellow-orange hue, suggesting an older stellar population and lower levels of ongoing star formation. Faint blue hints may be visible in the outer regions, implying the presence of younger, hotter stars, although the dominant stellar population appears to be evolved. No prominent spiral arms, bar structures, or dust lanes are discernible. The overall form is generally round, showing minimal deviation from a circular shape. There is no strong evidence of any ongoing or recent major mergers or tidal disturbances affecting the overall structure.
