The galaxy presents as a lenticular or early-type spiral galaxy with a prominent bulge and a faint disk component. The central bulge exhibits a yellowish hue, suggesting a population of older stars. The disk, though faint, appears bluer, hinting at younger stars and possibly ongoing, albeit low, star formation. The galaxy has a relatively smooth morphology, with no readily apparent signs of major disturbances, active galactic nuclei features, or ongoing merger activity. A subtle disk structure is visible upon close inspection. It is moderately sized.
