The galaxy presents as an elliptical or lenticular structure with a prominent, bright central bulge. The light from the bulge appears relatively smooth and concentrated. A fainter, more diffuse halo surrounds the central region, suggesting a gradual decrease in stellar density with increasing distance from the core. There may be a slight hint of a disk component, evidenced by a subtle flattening or extension along one axis, though this is not clearly defined. There is some evidence of minor disturbances in the structure, such as irregularities in the outer halo or faint tidal features, but the galaxy appears largely undisturbed. The overall color profile suggests an older stellar population, possibly with ongoing, albeit low, star formation.
