The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a smooth, concentrated morphology with no discernible spiral arms or prominent dust lanes. The central bulge is bright, and the overall structure appears largely spheroidal, with high degree of roundness. There is no apparent evidence of ongoing major mergers or significant tidal disturbances. The color index suggests a population of older stars, as the galaxy has a yellow-orange hue, with a high fraction of being smooth. Given the high degree of smoothness and roundness, this galaxy could be considered an early-type galaxy.
