The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The primary color of the galaxy is a yellow-orange hue, possibly indicating an older stellar population and lower rates of star formation. There are subtle color gradients visible, with the central region appearing slightly more yellow than the outer regions, suggesting possible variations in stellar age or metallicity. Based on the high degree of being smooth, disk-like features are not prominent. No significant tidal disturbances or signs of recent mergers are evident. The galaxy appears to be relatively isolated. Overall, the galaxy appears as a passively evolving system.
