The galaxy presents as a moderately bright, lenticular or early-type spiral system at a redshift of approximately 0.119. Its morphology is dominated by a smooth, centrally concentrated bulge that appears nearly spherical and possesses a yellowish hue. The disk component, while present, is subtle and exhibits a bluer color, suggesting the presence of some ongoing star formation. The galaxy lacks any obvious signs of major disturbances or ongoing mergers, and is reasonably isolated. Based on the subtle features in its disk it is a large system with a mass slightly over 10^10 solar masses.
