The galaxy presents as a relatively smooth, lenticular-like system with a high degree of central concentration. The morphology suggests a disk-like structure viewed at an oblique angle, showing elongation. The nucleus region exhibits a yellowish-white hue, indicating an older stellar population dominating the core. A faint blueish tint can be observed within the disk, potentially indicating ongoing, though subdued, star formation. There is a possibility of some disturbance due to other galaxies and gas in the area.
