The galaxy presents a largely smooth morphology, with an elliptical appearance. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars. Color gradients within the galaxy indicate potential variations in stellar populations. A subtle disk-like structure can be observed. The absence of significant tidal features suggests that the galaxy is not currently undergoing a major merger event. The moderate star formation rate estimates are consistent with the observed colors, indicating a galaxy that is neither intensely star-forming nor entirely quiescent. The overall shape suggests a classification as an early-type spiral galaxy.
