The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a concentration of light, appearing bright and somewhat yellow-green in color, possibly indicating an older stellar population. The light smoothly diffuses outward from the core, with no readily apparent spiral arm structures or distinct star-forming regions. There are no signs of major tidal disturbances, although there is a very slight asymmetry in the outer regions, suggesting a possible minor interaction or merger history.
