The galaxy presents as a somewhat elliptical, yet subtly disk-like structure with a smooth overall appearance. Its color profile exhibits a central concentration of yellow-orange hues, suggesting an older stellar population in the core. Moving outward from the center, the color gradually shifts towards a more blue-green tone in the outer regions, hinting at the presence of younger, hotter stars and potentially some ongoing star formation, however at a low rate. There is a hint of a possible disturbance or asymmetry in the outer regions on the left side. The galaxy appears fairly isolated, showing no obvious signs of interaction with any other nearby galaxies.
