The galaxy appears as a centrally concentrated, relatively smooth object. Its color is predominantly yellowish-orange, suggesting an older stellar population and potentially a lower rate of ongoing star formation. The galaxy exhibits a high degree of roundness. There's no clear evidence of spiral arms or a well-defined disk structure from this viewing angle and resolution. No significant tidal features, distortions, or other signs of recent or ongoing major mergers are visible. There might be a slight asymmetry in the outer regions, but this could also be due to image noise or minor interactions. Overall, the galaxy presents as an elliptical or lenticular galaxy viewed at a distance, with a generally relaxed morphology.
