The galaxy appears as an elliptical or lenticular galaxy with a relatively smooth morphology. The galaxy's light distribution suggests a higher concentration of stars toward its center, gradually decreasing in intensity towards its edges. The overall color is somewhat redder, indicating an older stellar population with relatively little ongoing star formation. The galaxy shows a slight elongation, appearing more cigar-shaped than perfectly circular. There is no clear evidence of significant spiral arm structure or major disturbances, although a minor disturbance cannot be ruled out. There are no distinct signs of a recent or ongoing major merger. The galaxy is relatively compact, with a size on the order of a few kiloparsecs.
