The galaxy appears to be an elliptical galaxy at a redshift of approximately 0.2, indicating a significant distance. The galaxy exhibits a smooth, spheroidal morphology, lacking prominent spiral arms or a distinct disk structure. The color profile suggests a population dominated by older stars, with a redder hue indicating less ongoing star formation. There is no evidence of significant tidal disturbances or ongoing mergers, suggesting the galaxy is relatively undisturbed. The galaxy's high degree of roundness indicates that it is viewed close to face-on.
