The galaxy presents as a relatively compact and smooth object, likely an elliptical or lenticular type. It appears mostly featureless, lacking prominent spiral arms or a distinct bar structure. There is a slight elongation, but the overall shape is quite circular.

The galaxy's color gradient suggests an older stellar population, with a concentration of redder hues toward the center, possibly indicating a higher density of older, cooler stars there. Some bluer patches are visible, implying that there is likely a younger stellar population existing within the galaxy. The galaxy shows no signs of active merging, although there might be slight disturbances visible.

The galaxy is of moderate size. It appears to be fairly isolated, lacking any other large galaxies in close proximity, suggesting it has evolved in relative isolation.
