The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical. The light distribution suggests a relatively old stellar population, with a yellowish hue dominating the central region, indicative of evolved stars. There's a subtle fading of light intensity from the core outwards, with no apparent spiral arm structure or significant dust lanes visible. The outer regions appear slightly less luminous and more diffuse. There are no indications of any major mergers or significant tidal disturbances affecting the main body of the galaxy. The galaxy appears to be fairly isolated and relaxed in its environment, with no close companions immediately obvious.
