The galaxy presents as a moderate redshift object. It is lenticular in appearance, displaying a smooth, elliptical profile with a high degree of central concentration. The galaxy exhibits a yellowish-orange hue, suggesting a dominant population of older stars and a relatively low rate of on-going star formation. There is no obvious dust lane or spiral arm structure visible in this image. The morphology suggests an evolved system, likely a galaxy at least 4.5 kpc across, with a significant stellar mass. A slight asymmetry is noticed, and there may be a possible minor disturbance in its overall shape. The general visual assessment supports the classification of this object as a fairly massive system with limited current star-forming activity.
