The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its overall shape is somewhat elliptical, tending towards a less-rounded, in-between profile rather than perfectly circular. Color gradients indicate a likely older stellar population dominating the galaxy's light output. The lack of clearly defined spiral arms or dust lanes reinforces the impression of a well-mixed stellar population. There might be very minor disturbances, but no major mergers are evident.
