The galaxy appears to be an elliptical galaxy with a smooth, concentrated central bulge. It exhibits a slightly elongated shape, transitioning towards a cigar-like morphology. There is a suggestion of potential tidal disturbances and a merger of another galaxy. Evident is a strong central concentration of older stellar populations, indicated by the orange-red hue, with a lower level of ongoing star formation. Hints of bluer regions can be seen, with the possibility of scattered younger stars. The light distribution is relatively even and generally featureless.
