The galaxy presents as a moderately luminous, elliptical or lenticular structure. Its light profile appears smooth and centrally concentrated, lacking distinct spiral arms or a prominent disk. The core exhibits a bright, yellowish-white color, suggesting a population of older stars. A gradual color gradient extends outward from the core, transitioning to a slightly redder hue in the outer regions of the galaxy. The overall shape is somewhat elongated. There is no obvious evidence of ongoing major mergers or significant tidal disturbances, although subtle irregularities cannot be ruled out. Given its apparent smoothness, color, and lack of disk features, this galaxy likely ceased forming stars a long time ago.
