The galaxy presents as a moderately bright, elongated object. Its morphology appears intermediate between elliptical and spiral, possibly a lenticular galaxy. The light distribution suggests a relatively smooth structure with a bright central region and a diffuse, extended halo. There are subtle indications of a disk-like component. Color gradients across the galaxy are subtle, with the core exhibiting a slightly yellower hue, possibly indicating an older stellar population. Hints of bluer regions may indicate some ongoing star formation, though subdued. No major disturbances or mergers are readily apparent, though some minor asymmetry exists. The overall impression suggests a fairly evolved galaxy with a moderate mass.
