The galaxy presents as a roughly elliptical structure with a luminous core. The morphology indicates properties of both a smooth elliptical galaxy and a disk galaxy. Its color profile suggests a mixture of stellar populations, with a central bulge exhibiting a yellowish-white hue, potentially indicative of older, less active stars. The outer regions possess hints of blue, hinting at the presence of younger, hotter stars and ongoing star formation, although at relatively low levels. The galaxy's shape is primarily intermediate between round and elongated. There's a slight asymmetry visible, possibly caused by a minor gravitational interaction or disturbance, but no major merger events are apparent. The galaxy appears relatively isolated, though subtle tidal features might exist upon closer inspection.
