The galaxy appears as a centrally concentrated, luminous object, likely an elliptical galaxy due to its smooth, featureless appearance. The core exhibits a high surface brightness, suggesting a dense concentration of stars. The galaxy appears relatively round, with a slight elongation. There is no indication of spiral arms or significant dust lanes. The outer regions of the galaxy gradually fade into the background, indicating a smooth stellar halo. There is no obvious evidence of a major merger event or strong tidal disturbances.
