This galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated luminosity profile. It has a generally round shape, showing little evidence of a disk structure or spiral arms. The galaxy's color index suggests a population of older stars, exhibiting a redder hue than galaxies with ongoing star formation. There are no visible signs of major mergers or significant tidal disturbances, though a minor interaction cannot be ruled out based solely on this image. Based on the smoothness and roundness of the galaxy it is likely an early-type galaxy. The galaxy presents with a stellar mass estimated to be quite high. A low star-formation rate appears consistent with the observed color and morphology.
