The galaxy presents as a relatively smooth object with an elliptical morphology. There is a bright central bulge, which appears roughly spherical and dominates the galaxy's luminosity. The outer regions of the galaxy fade smoothly, indicating a gradual decrease in stellar density with increasing distance from the center. No distinct spiral arms or bar structures are readily apparent. The galaxy appears to be relatively isolated, with no obvious signs of major interaction or recent merger events. Faint tidal features cannot be ruled out. The color profile suggests a population of older stars, possibly a relatively quiescent galaxy. The overall appearance is consistent with an early-type galaxy. 
