The galaxy presents as an elliptical or lenticular system, exhibiting a high degree of smoothness with minimal discernible features. The morphology is largely spheroidal, approaching a circular form in its projected shape. There is a slight yellowish tint to the light emanating from the galaxy. Based on the high smoothness fraction, a spiral structure is unlikely; any disk component is subtle or non-existent.

Evidence of merging or tidal disturbances is minimal. The object appears relatively isolated and relaxed in its current form. Based on the single image, further analysis would be needed to ascertain more refined morphological details such as the presence of a faint outer halo or tidal streams.
