The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular type. It exhibits a generally elliptical morphology with an apparent roundness, lacking strong indications of spiral arms or a bar structure. The color profile suggests a dominant older stellar population, as indicated by the redder hue in the central region, transitioning to slightly bluer colors in the outer regions, which may indicate the presence of younger stars. The galaxy shows no obvious signs of major mergers, though there is a slight asymmetry to its overall structure, which may indicate past interaction or minor disturbance. The observed magnitude suggests a luminous galaxy.
