The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth and featureless morphology. There is a subtle elongation, suggesting it is not perfectly spherical and has a slight cigar shape. The galaxy's color profile indicates a relatively evolved stellar population, with a dominant yellowish-red hue. While a central bulge is implied by the concentration of light, there is no visible evidence of active star formation regions or prominent spiral arm structures. There is no apparent major disruption or signs of an ongoing merger event with another galaxy, only hints of possible tidal disturbances.
