The galaxy presents as a largely featureless elliptical or lenticular type. The central bulge appears bright and concentrated, exhibiting a yellowish-gold hue indicative of an older stellar population. There is little evidence of spiral arm structure or dust lanes. The overall shape is largely spherical, with a slight deviation from perfect roundness. No signs of ongoing mergers or major disturbances are discernible, suggesting a relatively quiescent evolutionary state. The galaxy demonstrates a moderate degree of star formation.
