The galaxy presents as an elliptical or lenticular type, with a predominantly smooth light distribution, concentrated towards the center. The central bulge appears largely spheroidal and exhibits a yellowish-orange hue suggesting an older stellar population. The outer regions of the galaxy display a bluer color gradient, hinting at the presence of some younger stars or ongoing star formation. A faint tidal tail-like structure is observed on one side of the main body, possibly indicating a past interaction or merger event, this disturbance appears relatively minor. Overall, the galaxy appears largely undisturbed in its morphology.
