The galaxy presents as a relatively smooth, elliptical structure, exhibiting a moderate degree of elongation. Its core region is characterized by a bright, concentrated light, suggesting a high stellar density. There's a noticeable colour gradient from the centre outwards, transitioning from a yellowish core to a bluish outer halo. This color gradient may indicate a central concentration of older stellar populations, while the outer regions show evidence of ongoing star formation, even if at a low rate. No distinct spiral arm structures or significant dust lanes are readily visible. The overall morphology suggests a quiescent galaxy, potentially in the late stages of its evolution. There are no obvious signs of major interactions or mergers, although minor disturbances cannot be ruled out.
