The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. There is a noticeable color gradient, with the central region exhibiting a yellowish hue, suggesting an older stellar population dominated by evolved stars. The outer regions appear slightly bluer, possibly indicating the presence of younger stars, though the overall morphology suggests limited ongoing star formation. The galaxy appears to be generally isolated, without any obvious signs of tidal disturbances or interaction with other galaxies. While it is difficult to discern detailed internal structures, the overall appearance suggests a high degree of symmetry and order.
