The galaxy presents as a smooth, elliptical structure with a moderate redshift. It exhibits a pronounced cigar shape. There are no distinct spiral arms or a prominent disk visible; the light distribution appears relatively uniform across the galaxy. There is no evidence of recent or ongoing major merger activity, nor indications of strong tidal disturbances. The core of the galaxy appears slightly brighter than its outer regions, suggesting a possible concentration of older stellar populations toward the center. The overall color profile suggests a redder hue, consistent with a population of older stars.
