The galaxy exhibits a generally smooth morphology, with a dominant ellipsoidal shape. Its appearance is largely featureless, lacking defined spiral arms or a prominent central bulge. The light distribution is centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. The color gradient suggests a redder core, potentially indicating an older stellar population, transitioning to slightly bluer hues in the outer regions, indicative of younger star formation. The overall color index implies that the galaxy likely has a mixed population of stars. There is no visual indication of any significant tidal disturbances or mergers.