The galaxy presents as a luminous, centrally concentrated object. The core region exhibits a strong, yellowish-white glow, indicating a high density of older stars. The luminosity falls off gradually from the center, transitioning into a fainter, more diffuse halo or disk. The color of this outer region appears slightly bluer compared to the core, which may suggest the presence of younger stellar populations and ongoing star formation, although at a relatively low rate. The overall shape leans towards being somewhat elliptical, but not perfectly spherical, appearing slightly elongated or in between a round and cigar shape. There are no prominent spiral arms or distinct features readily visible, and it appears relatively undisturbed, showing no significant signs of a major merger event, though there may be a very subtle asymmetry hinting at a minor disturbance or past interaction. The galaxy is located at a considerable redshift.
