The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology with minimal discernible features. The central bulge appears prominent and displays a yellowish-orange hue, potentially indicating an older stellar population. A fainter, greenish halo surrounds the core, suggesting the presence of some younger stars or ionized gas, but the overall star formation activity seems relatively low. There is no evidence of spiral arms, a bar structure, or significant dust lanes. The galaxy appears largely undisturbed, with no signs of a major merger event or tidal distortions. Minor irregularities in the outer regions might suggest a past interaction.
