The galaxy presents a generally elliptical morphology, elongated along its major axis. It exhibits a smooth overall appearance, with a high degree of central concentration indicated by a bright, prominent nucleus. The light distribution appears to diminish gradually from the core outward, suggesting a relatively old stellar population. The colors observed suggest a mature galaxy with lower levels of active star formation. A slight asymmetry in the outer regions might indicate a past minor interaction or disturbance but overall shows no strong signs of ongoing merger activity, although the faintest hint of possible tidal features is present. The galaxy is not perfectly spherical, showing a slight cigar shape.
