The observed galaxy presents a generally smooth, elongated morphology, appearing as a cigar shape. The central region exhibits a concentration of light, suggesting a prominent galactic bulge or nucleus. The color gradient transitions from a yellowish-white core to a bluer, fainter outer region. There's a subtle indication of asymmetry, potentially suggesting a minor gravitational interaction or internal disturbance, though no large tidal features or obvious signs of a major ongoing merger are apparent. The overall structure appears relatively undisturbed, indicative of a system that has undergone primarily quiescent evolution. The angular size implies that we're likely viewing a significant galaxy at cosmological distance.
