The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The central region exhibits a bright, yellowish-white core that likely corresponds to a dense concentration of stars. The galaxy's overall shape appears roughly circular. There is no obvious evidence of spiral arms or a prominent disk structure. The outer regions of the galaxy fade gradually into the background, with no signs of significant tidal features or major disturbances, with possible minor disturbances. There's no evidence of any major mergers. The color gradient suggests an older stellar population.
