The galaxy presents as a concentrated, yellowish, elliptical-shaped object. Its morphology appears largely smooth with a high degree of central concentration. There is no prominent disk or spiral arm structure visible. The main body of the galaxy exhibits a gradual decrease in luminosity from its core outward. There is a subtle elongation; however, the object's shape is mostly round. No significant signs of tidal interactions or merging activity are immediately apparent, though some minor disturbances cannot be entirely ruled out. The overall color suggests an older stellar population.
