The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. The galaxy's color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region, potentially indicating a higher concentration of evolved stars. The overall shape seems elongated or cigar-shaped, displaying a slight deviation from perfect sphericity. There is no visual evidence of significant tidal disturbances or ongoing mergers. The galaxy appears relatively isolated, with no immediately apparent interacting companions. Based on its overall appearance, this galaxy likely ceased significant star formation some time ago.
