This galaxy presents as an elliptical morphology, exhibiting a smooth, featureless structure. It appears moderately elongated, with an axis ratio suggesting a classification between E4 and E6 on the Hubble sequence. The central region displays a concentrated luminosity, gradually decreasing towards the outer edges. The color gradient indicates a redder core, transitioning to slightly bluer hues in the outer regions. Faint distortions may be present in the galaxy's disk indicating possible minor disturbances due to a past interaction, though there is no major merger event. The overall shape is consistent with a galaxy undergoing slow star formation, potentially evolving towards a more passive state.
