This galaxy appears to be a relatively smooth, elliptical-type galaxy. The main body of the galaxy exhibits a diffuse, fuzzy morphology, with a moderately concentrated central region. There is a slight elongation. There also appears to be a few faint objects in the vicinity, possibly representing tidal debris or dwarf galaxies. These could indicate past or ongoing merger activity. The galaxy shows subtle color variations across its body with the central region exhibiting redder hues than the surrounding areas. This could be indicative of an older stellar population in the galactic core. The presence of possible disturbances suggests that, despite its generally smooth appearance, this galaxy has a complex dynamical history.
