The galaxy presents as a single, prominent object. Its morphology suggests a relatively smooth, elliptical structure with a high degree of central concentration. The light profile appears to follow a Sersic model, with a notable deviation from a simple exponential disk or bulge. There is an indication of a slight elongation, and a small degree of flattening of the galaxy is apparent. The primary color of the galaxy is somewhat redder than the surrounding space, indicating it may be older and the star formation rate is low.
