The galaxy presents as a smooth, elliptical structure with a moderately elongated morphology. The central region exhibits a concentration of light, appearing yellowish, suggesting a population of older stars. The outer regions show a gradual decrease in brightness, with a subtle bluish tinge, potentially indicating a small amount of recent star formation. There is no apparent dust lane or spiral arm structure. The galaxy appears to be relatively isolated, showing no signs of major tidal disturbances or interaction with other galaxies.
