This galaxy presents as a relatively smooth, elliptical or lenticular system at a redshift of approximately 0.21. Its morphology is largely spheroidal with a highly concentrated central bulge exhibiting a yellowish hue, indicative of an older stellar population. There's little evidence of prominent spiral arms or significant dust lanes. The light profile fades smoothly from the core, transitioning into a faint, diffuse halo. The overall roundness suggests a low degree of intrinsic flattening. Minor disturbances or merger activity is not apparent based on visual inspection.
