The galaxy presents a roughly elliptical morphology, appearing relatively smooth in its overall structure. A bright, concentrated central bulge is visible, indicating a high stellar density in the core region. Diffuse light extends outwards from this central region, suggesting the presence of a surrounding disk or halo. Hints of bluer regions suggest the possibility of some on-going star formation, although this appears relatively subdued. Some disruption can be observed, it is unclear whether this is due to a small merger or another gravitational interaction.