The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its core appears bright and yellowish-orange, potentially indicating an older stellar population. The galaxy exhibits a slight elongation, with the shape tending toward "in-between" round and cigar shaped, lacking distinct spiral arms or disk-like features. There's no obvious signs of active merging or major disturbances, though the subtle asymmetry might suggest some past interaction.